BOND DISSOCIATION ENERGIES IN SULPHUR ORGANIC COMPOUNDS •·" • BOND DISSOCIATION ENERGIES IN SULPHUR ORGANIC CO~OUNDS by Robert L. Lauchlan, B.Sc. A thesis submitted to the Faculty of Graduate Studies and Research in· partial fulfilment of the requirements for the degree of Doctor of Philosopny. Department of Chemistry, McGill University, Montreal. October 1965. • AOKNOWLEDGEMENTS The author wishes to acknowledge the guidance of Dr. A. Sehon in the supervision of this research and in the preparation of the manuscript. Mr. S. Meyerson of the American Oil Company, Whiting, Indiana, contributed mass spectroscopi e analyses,· providing the author invaluable assistance. Grants from the Petroleum Research Fund of the Ameriean Chemical Society and the National Research Oouncil of Canada made to Dr. A. Sehon in support of this research are gratefully acknowledged . The author is deeply indebted to his wife for the editing and typing of this manuscript. TABLE OF CONTENTS Introduction 1 Factors Affecting Bond Dissociation Energies 7 Methode of Measuring Bond Dissociation Energies 18 Spectroscopie Methode 19 Electron Impact Methode 23 Thermal Methode A. Equilibrium Methode 28 B. Kinetic Methode 34 Carbon-Sulpnur Bond Dissociation Energies Review 47 Present Investigation 51 Experimental 54 Materials 54 Apparat us 54 Procedure and Analyses 61 Resulte and Discussion A. B. 67 Phenyl Ethyl Sulpnide Products 67 Mechanism of Decomposition 72 Bond Energies 78 Phenyl n-Propyl Sulpnide Products 88 Mechanism of Decomposition 89 TABLE OF CONTENTS (cont.) Bond Energies C. 94 Phenyl Benzyl Sulphide Pr~oo~ 1~ Mechanism of Decomposition 105 Bond Energies 106 General Discussion Experimental Errors 111 111 Dissociation Energies and Heats of Formation of Radicals 112 The Stability of the Pheny1sulphide Radical 115 Appendix A Pyrolysis of Diphenyl Disulphide 116 Appendix B Data and Calculations for Experiment 20 121 Summary and Contributions to Knowledge 123 Bibliography 126 !NDEX TO F IGJ.Jl\ES 1. 2. Graphie representation of bond dissociation energies and ionie-covalent resonance 14 Appara tus 58 3A. Section of apparatus for the introduction of liquid su1phides 59 3B. Section of apparatus for the introduction of solid sulphides 59 4. Reaction Vessel 60 5. Titration curves for mercaptans 69 6. Titration curves for su1phides 70 7. Separation of ethane and ethylene on column of high activity silioa gel by gas ohromatography 8. Plot of log k vs. 1/T (pheny1 ethyl sulphide) 9. 71 81 Plot of log k vs. 1/T (phenyl n-propyl sulphide) 98 10. Plot of log k' vs. 1/T (phenyl benzyl sulphide) 108 INDEX TO TABLES 1. Bond dissociation energies and bond energy terrns 6 2. C-H bond dissociation energies in hydrocarbons 8 3. Dissociation energies of RX bonds 12 4. Dissociation energies of the metal alkyls 16 5. Primary C-S bond dissociation energies 49 6. Products of the decomposition of phenyl ethyl sulphide 7. 82 The decomposition of phenyl ethyl sulphide Variation of k with contact time 8. 83 The decomposition of phenyl ethyl sulphide Variation of k with the partial pressure of 84 sulphide 9. The decomposition of phenyl ethyl sulphide Variation of k with toluene pressure 85 10. The decomposition of pnenyl ethyl sulphide Effect of the packed reaction vessel on k 86 11. A comparison of abstraction and decomposition reactions for C2H5 12. Products of the decomposition of phenyl 87 n-propyl sulphide 99 13. The decomposition of phenyl n-propyl sulphide Variation of k with contact time 100 ~~ ~ -- ~~~~~~~--~~~~--- INDEX TO TABLES (cont.) 14. The decomposition of phenyl n-propyl sulphide Variation of k with the partial pressure of sulphide 101 15. The decomposition of phenyl n-propyl sulphide Variation of k with toluene pressure 102 16. The decomposition of phenyl n-propyl sulphide Effect of the packed reaction vessel on k 103 17. Products of the decomposition of phenyl benzyl sulphide 109 18. Products of the decomposition of phenyl benzyl sulphide in toluene-J:-d llO disulphide 120 3 19. Products of the decomposition of diphenyl INTROIUlCTION In a discussion of the strengths of ohemioal bonds it is important to distinguish between two concepts, the 'bond dissociation energy' and the 'bond energy term'. Since chemical reactions involve the formation and rupture of bonds, it is clear that bond dissociation energies must be considered among the main determining factors of chemical reactivity. However, bond properties, auch as the bond length, are more effectively correlated with the bond energy term which representa that fraction of the total molecular binding energy that can be ascribed to a particular bond as it exista in the undisturbed molecule. The bond dissociation energy, as a pbysical concept, has a great advantage over the bond energy term, since it can be defined without ambiguity. Szwarc (1) has defined the bond dissociation energy, D(A-B), of a bond A-B as the change· ih internai energy at absolute zero, .6E~, in the ideal gas state for the reaction A-B ~ A+B (1) the products existing in their ground states or specified electronic states. Dissociation energies derived from spectral data refer to absolute zero, but those derived - 2 - from equilibrium or kinetic data often refer to the temperature used in the particular experimenta, since the necessary heat capacity data required to make the correction to absolute zero are frequently lacking. 0 0 Cottrell (2) has shawn the difference, AH2gs - AE 0 to be about 4RT, a value which is well within the experimental error involved in bond dissociation energy measurements. In contrast to bond dissociation energies, the bond energy term cannat be defined with complete precision except in the restricted case of a diatomic or symmetrical polyatomic molecule. The sole criterion of correctness in apportioning the total energy of a molecule among the various bonds is that the sum of all its bond energy terms is equal to the heat of atomization, H:. The simplest scheme, as proposed by Fajans (3), assumes a theory of local pair bonds without interaction between bonds. Each bond of a given type has a constant energy term, irrespective of the molecular environment, and all bond energy terms are additive. For a molecule ABn containing only A-B bonds, the bond energy term is then defined as 1/n the heat of atomization of the gaseous molecule at 298.15°K. (2) - 3 Applied to methane, this definition gives a value of E(C-H) = 99.29 kcal./mole (4). However, the extension of equation (2) to the evaluation of E(C-H) and E{C-C) terms in the straight-chain paraffin hydrocarbons leads to various values depending on which members of the series are compared. For example, the heats of atomization of butane and pentane give a value of E(C-H) = 98.70 kcal./ mole, which is slightly lower than the value calculated for E(C-H) in methane. In addition, this bond energy scheme fails to account for the significant differences in the heats of formation of isomers such as 1:4-pentadiene and 1:3-pentadiene (5), and erroneously classifies all gaseous redistribution reactions as thermoneutral (6). The initial proposal by Zahn (?) that interaction between localized bonds within the same molecule is significant received theoretical support from studies by Dewar and Pettit (8), who used the perturbation theory for their ca1cu1ations, and by Brown ,(9), who emp1oyed the 1inear combination of bond orbitals approximation. \ Severa1 authors have subsequently proposed schemes which differ from that of Fajans in at 1east one of the initial postu1ates. Laid1er (10,11) has accounted for the heats of formation of paraffin hydrocarbons in terms of a scheme which assumes that the strength of the C-C bond is constant, - 4 but that of the C-H bond varies according to whether it is primary, secondary, or tertiary. Tatevskii (12) has extended this classification to include c-c bonds. Similarly, Dewar and Schmeising (13) devised a scheme for olefine in which the term values for different types of C-H and C~C bonds are classified according to the state of hybridization of the carbon atoms involved. Bond energy terms in general have been criticized (14) as being unrealistic since the atoms in molecules, particularly in the transition state, seldom exhibit the same valence as in their ground state. The role of the valence state cannat, however, be ignored in the evaluation of dissociation energies. This is the prin- cipal reason not only for the difference in the energies of the stepwise dissociation processes of a polyatomic molecule but also for the difference between these values and the corresponding bond energy terms as shawn in Table I. For example, the C-F bond dissociation energies in tetrafluoromethane are neither constant nor equivalent to the bond energy term. Values of D(CF 3-F) : 123 kcal./mole (15) and D(CF-F) • 120 kcal./mole (16) have been estab- lished from electron impact and predissociation etudies, respectively. uncertainty exista in the evaluation of the final dissociation energy, D(C-F), although a value of llO - 5 - kcal./mole is consistent with available data {16). These values require that D(CF 2 -F) be 110 koal./mole, determined as the difference between the sum of the ether three bond dissociation energies and the heat of atomization of the molecule. Previous unoertainties (17) in the stepwise dissociation energies in hydrogen sulphide have been resolved and the values of D(HS-H) = 92 koal./mole (18) and D(H-S) = 81.4 kcal./mole {19) have been determined from thermoohemical and spectroscopie data. In general, bond dissociation energies have not been used as frequently as bond energy terms in estimating thermochemical quantities sinoe they are both diffioult to measure and sensitive to their partioular molecular environment. - 6 - Table I Bond Dissociation Energies and Bopd Energy Terms E(A-B) References Molecule lh ll2 HgC12 81 25 53 (20,21) HgBr2 72 16 44 (20,21) Hgi2 61 8 35 (20,22) 102 87 124 80 99 {23) 123 110 120 110 116 (15,16) TiC1 4 80 101 106 124 103 {20, 24) SH2 92 81.4 87 (18,19) OH2 117.5 101.5 110 NH3 103 92 85 93 91 95 119 102 CH CF 4 4 A1C13 ll3 (2) (25 ,26) (20) - 7 - Factors Affecting Bond Dissociation Energies The bond dissociation energy is equivalent to the difference between the heats of formation of the fragments and the heat of formation of the parent molecule or radical, (3) and is thus influenced directly by factors which affect any one of these terms. In order to avoid the ambiguities which result in the evaluation of molecular resonance energies from bond energy terms, Szwarc (27) defined the experimental resonance of a radical in terms of dissociation energies. resonance energy, ~' The experimental of the radical formed upon dissocia- tion of the molecule, RH, was defined as the relative lowering of the bond dissociation energy with respect to the value of D(OH -H) when a methyl radical is formed by 3 the dissociation of methane (4) Table II shows the lowering of the OH bond dissociation energies in a series of hydrocarbons. - 8 - Table II C-H Bond Dissociation Energies in Hydrocarbons Hydrocarbon Bond (R-H) Dissociation Energy AHr(R) Rr CH -H 3 102 32 0 (23) C2Hs-H 97 25 5 (23) n-c 3a,-H 99 22 3 (28) s-C 3Ry-H 94 17 8 (28) t-C 4H9-H 89 5 13 (5) C 6 H C~-H 80 40 22 (29) 77 29 25 (30) c 6H -H 5 102 70 (5) H2C:CH-H 105 65 (31) 5 2 H C:CHC~-H References - 9 - The resonance energies of the alkyl radicals were attributed to ~ -hyperconjugation (32); the greater the number of appropriate valence bond structures, the greater will be the resonance energy of the radical. analogy, By n -conjugation accounts for the large resonance energies associated with the allyl and benzyl radicals (33). The parent molecule might be subject either to stabilization from affects such as 1T-conjugation and ioniecovalent resonance, or to destabilization as a result of the release of 'reorganization' energy associated with reduction in steric strain or change in valence state. The reduction in length of the central c-c bond in 0 butadiene to 1.47 A from the 'normal' C-C bond length of 0 1.54 A has been attributed to lT-conjugation (34), although the extent of this affect has recently been questioned by Dewar and Schmeising (13). central c-c A parallel strengthening of the bond is reflected in the bond dissociation energy, D(C 2H3-c 2H3 ) = 104 kcal./mole, calculated by the combination of AHf(C2H 3 ) = 65 kcal./mole (31) with the appropriate thermochemical data. about 20 kcal./mole than the c-c This value·is larger by bond in ethane. A calculation of the central C-C bond dissociation energy in diphenyl from the beats of formation of the phenyl radical (35) and diphenyl (36) gives the value - 10 - D(C6H5-c 6H5 ) = 99.5 kcal./mole. This strengthening of the c-c bond by about 16 kcal./mole, with respect ta the c-c bond in ethane, can be attributed to TT-conjugation, the total effect of which bas been reduced due to steric interaction between four of the hydrogena which prevents complete planarity in the molecule (37). Combination of the heats of formation of the benzyl radical (29) and dibenzyl leads ta a value of 49.5 kcal./ mole for the dissociation energy of the central C-C bond in dibenzyl. If the weakening of the C-C bond were attributed solely ta the high resonance energy of the benzyl radical, then the bond dissociation energy should be lesa than that in ethane by 2 x 22 kcal./mole, giving a value of 39 kcal./mole. This strengthening of the bond has been attributed ta the partial double bond character resulting from hyperconjugation (38). A parallel 0 shortening of the C-C bond length ta 1.48 A (39) provides independant support for this conclusion. Szwarc (38) proposed that the extra weakening of the central c-c bond in hexaphenylethane ta the value of 11 kcal./mole was due not only ta resonance energy associated with the tripnenylmethyl radicale produced upon dissociation, but also ta steric repulsion between the two radicale. The activation energy required for the recombination of - 11 - triphenylmethyl radicale has been measured by Ziegler (40) as 8 kcal./mole, and may be considered to give an approximate measure of' the contribution of steric hindrance to the bond weakening in hexaphenylethane. The effect of the ionie character of a bond on the bond dissociation energy was initially discussed by Pauling (41) for diatomic molecules. It was proposed that the energy of a 'normal' covalent bond between atoms A and B be represented by either the arithmetic or geometrie mean of the experimental dissociation energies of the bonds A-A and B-B. The difference between the observed bond dissociation energy and that of a normal covalent bond between the same atoms was defined as the ionie-covalent resonance energy of the bond. Rie = D(A-B) - i( D(AA) + D(BB) ) (5) Baughan, Evans and Polanyi (42) employed the valence bond method in a consideration of ionie-covalent resonance in alkyl halides. In Table III the dissociation energies, given in kcal./mole, of various organic halides are compared with the corresponding hydrocarbons. - 12 Table III D~ssooiation Energies of RX Bonds References lm!: CH3 102 81 68 54 (28) C2H5 <J7 80 67 53 (28) n-C 3H7 99 82 68 54 (43) (CH3) 2CH 94 82. 68 53 (43) (CH3) 3c 89 78 64 48 (43) C6HsC~ 80 68 51 39 (43) This relative strengthening of the RX bonds in the series of alkyl halides has been attributed to the increase in ionie-covalent resonance energy in the molecule, and thus, to the increased stability of the R+x- ion pair. The resonance stabilization of the carbonium ion, R+, increases with the number of increasing valence bond structures and, therefore, with the number of carbons in the alkyl radical. There are thus two opposing factors which influence bond - 13 dissociation energies in alkyl halides. The radical resonance energy, Rr, tends to deorease the bond energy, whereas the ionie-covalent resonance energy of the molecule, Rio' tends to strengthen the bond. The difference, ARia' between the ionie-covalent resonance energies of the molecules RX and CH3X is defined by (6) ARia • D(R-X) - D(CH3-X) + Rr Figure 1, reproduoed from Baughan, Evans and Polanyi (42), shows the potential energy of the configuration R-X as a funotion of the interatomio distance. The full ourves Hii' Hoc' and E, represent the energies of the ionie, covalent, and ground states, respectively. The curve for the ionie state refera to the R+x- ion pair since for halides the curve representing the n-x+ ion pair lies sufficiently above the others to render contribution to the energy of the molecule negligible. The broken curves, Hii*, H00 *, and E* refer to configurations in whioh either the io.n R+ or the radical Ris resonance stabilized. The value for D(CH3-x) is greater than that expected for a purely covalent speoies by an amount, Rie' equivalent to the ionie-covalent resonance energy in the CH x molecule. 3 If the radical R in the molecule RX is resonance stabilized, then the aseymptotic energy value will be lower than that for CH3X by the radical resonance energy Rr• However, if - 14 - Figure 1 Graphie representation of bond dissociation energies a!]d ionie-covalent resonance. ' ' \ \ \ D(R-X) \\~J~''-----------·-A~~~tc_:____l_ INTERNUCLEAR DISTANCE . •. ~ :'u · 'llo;* · ,.,;, .,,,.:,,,_ •.. · ~- ( :. , . . . . . . . . . u."'~q,,,n:.ntA<.t-eÎuœ.i;. .,~~~!i'*"'•Alillidliii'Jiii1Aïu<e"'"'w.lii"":+I«m,!'!!!f<u."- N _;_ill'•...,..u ... ... - 15 the ionie-covalent resonance is more effective in RX than in CH ~, 3 then the ground state for RX will be lower than that for CH:;X by an a.mount, Ll.Ric' equivalent to the difference in resonance energies in the two molecules. The Rie values of 9, 5, and 7 kcal./mole as calculated by use of the equation (6) for benzyl chloride, bromide and iodide, respectively, demonstra.te the effect of ionie-covalent resonance on the bond dissociation energy. The relationsh~p between the bond dissociation energies of the metal alkyls and the valence state excitation energy of the metal atom has been discussed by Skinner (44). If the dissociation energies for the process . MR + R M+ R are represented as D1 and D2 , res pee ti vely, then reference to Table IV shows that D1 is greater than n2 , and that the differences n1 -D 2 are not constant. - 16 - Table IV DissociAtion Energies of the Metal Alkyle lll-~ References 8 43 (45) 42 8 34 (46) Hg (i-c3a, )2 27 15 12 (47) Cd(CH3 ) 2 45 22 23 (48) Zn (CH ) 3 2 47 35 12 (49) Molecule Dl ~ Hg(CH ) 2 3 51 Hg(C2H5)2 The bond in the molecule MR, where M is metal, is beat described by a wave function consisting of'terms for covalent, ionie, and non-bonding structures. The valence state energy of the atom, M, in a . li covalent bond M -R is dependent upon the nature of the hybrid orbitals, h 1 and h 2 , formed by the two valence electrons. ~ese orbitals are not necessarily equivalent hybrida, although the bonding orbital h 1 will assume that admixture of s- and p-character which resulta in the - 17 strongest bond relative to the excitation energy required. However, due to the non-bonding term, the 'effective' valence state energy will be somewhat less than that required to promote the atom M from the zero to divalent 1 state. The!bond dissociation energy, n2 , is therefore lowered by an amount comparable to this transition. The 'effective' valence state energy of the atom M in MR2 will be different from that in MR not only because the orbitais are then equivalent sp hybrida but also because the contributions from ionie and no-bond structures will differ. This may partly explain the variation in the differences (Dl-D2) • Pilcher and Skinner (50) have calculated the valence state excitation energies for the compounds TiC1 ,· TiC1 , 4 3 TiC1 2 , and TiCl by determining in each instance that particular hybrid obtained by mixing d3s and sp3 which resulta in the maximum orbital strength. Bath the valence state excitation energies and the ionization potentials of the titanium atom were found to deorease in the sense >TiC1 2 ) TiCl. The deoreasing ionization 3 potential signifies an inoreasing ionie character along the TiC14 > TiC1 series, as indicated by the deorease of p-character from 9/8 8/27 p in TiCl4 to p in TiCl in the isovalent configuration. Bath the diminishing valence state energy and the increasing - 18 - ionie-covalent resonance tend to increase the bond dissociation energies in the same sense D1 < D2 <D3 (D 4 as observed experimentally (24). Methode of Me~suring Bond Dissociation Energies Bond dissociation energies may be estimated directly by measuring the amount of energy involved in either the bond fission or bond formation processes. Measurement of the heat of recombination of atoms or radicals provides the only feasible method of determining the energy liberated in bond formation. Bichowsky and Copeland (51) obtained a value of D(H-H) = 105 kcal./mole from a measurement of the hea.t of recombina.tion of hydrogen atoms by direct calorimetry. The atoms were initially generated by electrical discharge and subsequently recombined catalytically in a platinum calorimeter. was estimated by the effusion method. Their concentration However, an extension of the method to the recombination of oxygen atoms resulted in high values for the 0-0 bond dissociation energy (52), perhaps due to the participation of metastable oxygen atoms in the recombination reaction. Studies of bond fission have proved to be more profitable in the evaluation of bond dissociation energies, the methods employed being classified according to the mode in - 19 which the energy of dissociation is supplied. P.h.oto- chemical msthods include those in which energy is supplied in the form of radiation, such as absorption spectra and predissociation Pbenomena. Electron impact studies utilize the kinetic energy of a beam of electrons to dissociate and ionize molecules. Thermal and pyrolytic methode may be divided into equilibrium and kinetic studies. Whereas, the former allows the calculation of the heat of dissociation from data based on the equilibrium between the undissociated molecules and the fragments derived from the bond fission, the latter leads to the determination of the activation energy for ~e dissociation process based on the kinetics 1 of the bond!breaking reaction. Spectroscopie Methods The sp,ctroscopic determi~ation of the dissociation energy of a'molecule requires a knowledge both of the energy of a dissociation limit above the ground state and of the state of excitation of the products of dissociation at this limit. When a band convergence with its adjoining continuum is observed lin absorption, the dissociation limit of the upper state can be accurately evaluated. In the case of - 20 - iodine, it can be shawn (53) that at the convergence limit dissociation takes place into one normal atom 2 2 in the P3; 2 state and one in the metastable P 112 state. Since dissociation energies refer to a~oms in their grounà state, D(I2 ) will be lees than the dissociation limit of the upper state by an amount equivalent to the energy of excitation of the state. 2 P1; 2 Similar spectra have been used to determine dissociation energies of bromine (54) and oxygen (55). For the numerous cases in which no band convergence is observed, Birge and Sponer (56) proposed that an approximate value for the dissociation limit can be obtained by an extrapolation from observed bands. The dissociation energy in a given electronic state is equal to the sum of all the vibrational quanta D (A-B) = L v AG(v + 1/2) and can therefore be approximated by the area under the h.G · curve in a plot of the vibrational quanta .â G against the vibrational quantum number v. extrapolation of the ~G Although a linear curve to eut the v axis gives values that represent an upper limit for the dissociation energies of non-polar molecules, more ac cura te extra-polation methods (57) can be employeà if sufficient vibra- - 21 - tional quanta are obeerved to detect the curvature of the ~G curve. A Birge-Sponer extrapolation gave a value of 81.4 kcal./mole (19) for the dissociation .energy of the hydrosulphide radical, in reaeonable agreement with that evaluated thermochemically. When a continuoue spectrum is observed without the accompanying band structure, the long wavelength limit of the continuum gives an upper limiting value for the dissociation limit under consideration. The most accurate value for hydrogen was determined in this way (58). The diffuseness of certain band spectra and the breaking off in the rotational structure of some emission bands can often be attributed to predissociation. This effect is due to a radiationless transition from a discrete electronic state to a continuous state at the same energy, with a resultant spontaneous decomposition of the molecule. The degree of diffuseness resulting from pre- dissociation is determined by the Kronig selection rules and the Franck-Condon principle. The ons et of diffuse- ness gives an upper limiting value for the dissociation limit of the state causing the predissociation. This method was used to determine dissociation energies for nitrogen (59), sulphur monoxide (60), and sulphur (25). - 22 When a continuous or diffuse absorption spectrum corresponds to dissociation into a normal and excited atom, then the absorption process may be followed by the emission of a corresponding atomic line in fluorescence. The long wavelength limit for the appearance potential of the atomic fluorescence gives an upper limiting value for the dissociation limit. Terenin (61) has applied this method to the alkali halides. The longest wavelength of incident light that will cause pnotodissociation gives an upper value for the dissociation limit. In this way, Flory and Johnston (62) attributed the photodissociation observed when irradiating 0 . nitric oxide with the mercury line 1832 A to predissociation and thus established an upper limit of 6.77 ev. for D(N-0). Ambiguities that e:xist in dissociation energies derived from spectr0scopic data arise chiefly from uncertainties in the state of excitation of the products. However, in cases where the Wigner-Witmer correlation rules fail to differen-tiate between several sets of allowed atomic states resulting from a particular molecular state, it is often possible to select the true atomic state if an approximate value for the dissociation energy is known from thermochemical evidence. An exact value of the dissociation energy - 23 can then be determined. For example, from the observed predissociations, three values for D(S ), 76.1, 83.0, 2 and 101.5 kcal./mole, are possible depending on whether it is assumed that bath the atoms are in the normal 3P state or one in the 3P state and one in the excited 1D state. The approximate value of 97 ± 5 kcal./mole recently obtained by Colin et al. (63) from mass spectrometric measurements on the vapour pnase above calcium sulphide supports the highest value for D(S 2 }. Electron Impact Methode The iDjteraction of mono-energetic electrons with molecules often resulta in molecular dissociation and ionization. The fragment ions produced are characterized by their maas-charge ratios in a mass spectrometer. The minimum electron energy at which a fragment ion is just produced, referred to as the appearance potential, is measured by the accelerating potential of the electrons at which the appropriate ion current first appears. For the· process in which a positive ion and a neutral fragment are generated R1~ + e ---+- R1 + + ~ + 2e the appearance potential, A(R1 +), of the ion R1 + is related to the dissociation energy and the ionization potential, - 24 I(Rl), of radical R1 by the equation . + ACl\1 ) = D(R1 - R ) + I (R1 ) 2 provided t~t no excess energy or activation energy is i~ involved In the process. gen~ral, electron impact experimenta on poly- atomic molecules have been interpreted on the assumption that radica~s and radical ions produced are in their respective ground states. For example, the cyanide radical formed in electron impact etudies on cyanogen was considered to be in the excited (A21T i) state. On this basis, Stevenson (64) rejected the value D(NC-CN) 6.90 ev. in favour of the lower value 4.64 ev. 1 = However, a subsequent study of the reaction of grapnite with nitrogen at·2500°K by Berkowitz (65) established a value of D(NC-CN) = 6.20 ev., which correlates with a cyanide radical in the ground state in electron impact. If R1 is an atom, its ionization potential is known from spectroscopie measurements. However, when R is a 1 complex free radical, the ionization potential must be determined by an electron impact method. Stevenson (~6) Hipple and combined the directly measured ionization potentials of the methyl and ethyl radicals with the appearance potentials of these ions from methane and ethane to obtain values of 4.44 and 4.23 ev., for D(CH3-H) and - 25 D (C 2Hs-H), :respectively. These values correspond to heats of formation of 32 and 25 kcal./mole, respectively, for the i me~hyl and ethyl radicals. Since ldirect measurement of the ionization potentials of free raqicals is difficult experimentally, it is often easier to dbtain bond dissociation energies indirectly by calculation from appearance potentials. Stevenson (67) and Hipple and Stevenson (66) have shown that, by measuring the appeara~ce potential of R + from R R and R H, in 1 2 1 1 conjunction with appropriate thermochemical data, D(R2 -H) 1 can be calciulated. Addition of A2 and R2H 1 3 and subtraction of A1 gives ~ R +H D(R2 -H) 2 ~H Using this method Stevenson measured A(0 2HS+) = 15.2 ev. from ethane and 14.5 ev. from propane and, in combination re~uired heats of formation, evaluated D(OH -H) 3 4.38 ev., in excellent agreement with the value measured with the directly. Electron impact studies on thiols, sulpnides and di- = - 26 sulPhides have provided much of the available information on S-H, c-s, and S-S bond dissociation energies and the heats of formation of sulphur organic radicale. and Lumpki~ Franklin (68) studied the process ~H+e R+ + SH + 2e for the ethyl, n-propyl, and t-butyl mercaptans, deriving a value of 38 kcal./mole for the heat of formation of the hydrosulphide radical, based on measurements of th~ c2H +, 5 + + n-c 3H? , and t-c H ions from the corresponding mercaptans. 4 9 In the light of more recent information, Mackle (18) reinterpretbd the data for the ethyl mercaptan system and arrived at a va~ue of AHf(SH) = 35.2 ± 4.5 kcal./mole. From a similar study of the process SH+ + H + 2e Palmer and Lessing (69) derived a value of ~Hf(SH) : 33.7 + 3 kcal./mole based on direct measurement of the ionization and appearance potentials of the hydrosulPhide ion. Both values agree, within the limita of experimental error, with the value of 34.9 ± 4.5 kcal./mole derived by Sehon and Darwent from the study (70) of the pyrolysis of benzyl mercaptan. Palmer and Lessing (69) also determined the heat of formation of the methyl sulPhide radical indirectly from measurements of the appearance potentials 1 of the radical ion formed from methyl sulPhide and dimethyl - 27 disulphide · . ! CH3sqH3 + e CH3SSCH + e 3 The value o1f .llHf(SCH3 ) the equation CH + SCH + + 2e 3 3 CH s + SCH + + 2e 3 3 = 31.8 kcal./mole evaluated from is in agreement with the value 30.5 ± 5 kcal./mole based on the pyro}ysis of benzyl methyl sulphide by Braye et al. (71). Although improved techniques for producing monoi energetic electrons have simplified the -problem o:f deter- mining appearance potentials, the interpretation of these appearance potentials in terms of bond energies requires an exact knqwledge of the fragmentation process. The va\ue for the ionization potential of the benzyl radical as d~termined directly is at variance with the value determined from appearance potentials. Schissler and Stevenson (72) derived a value of 8.51 ev. for the ionization potential of the potentials e~aluated ethylbenzene~ c7H7 radical based on the appearance :from the mass spectra of toluene, and dibenzyl. However, Lessing and his co- workers (73) obtained the lower value of 7.76 ev. from - 28 - direct measurement of the ionization potential of radicale produced from toluene. c7H? Combined with the appearance iPOtential from toluene these ionization values of D(C 6H5CH2-H) = 77 and 95 kcal./ mole, the former being in agreement with Szwarc's value potentials ~ive 77.5 kcal./mole (74). Howeve~, the appearance potential of the c7H?t ion depends upo~ the structure of the parent ion before fragmentation. Rylander, Meyerson and Grubb (75) proposed i the rapid rearrangement of the parent ion from toluene to form the symmetrical cycloheptatriene molecule-ion with subsequent decomposition to yield a stable tropylium ion plus a hydrogen atom. The higher value for the C-H bond dissociation energy of toluene as measured directly could be explained if the appearance potential of the tropylium ion were higher than that of the benzyl ion. Thermal Methpds A. Equilibr!um Methode i Bond dissociation energies, as determined by the equilibrium method, are based on the measurement of the equilibrium constant for the dissociation reaction 1 AB ... . A+ B - 29 The equili~rium constant can be evaluated by either the second or third law of thermodynamics. 1 1 of the equ~librium Knowledge constant over a range of tempera- tures allows calculation of the heat of dissociation ' from the van't Hoff equation d ln K dT = AR~ from which .AH~ can be ca.lculated if the relevant heat capacity data are known. From a knowledge of the equili- brium constant at a single temperature and of the appropriate'free energy functions for the reactants and products, the heat of dissociation can be evaluated by the third law method 0 - R ln K = .6Ho t T 0 " 0 .6(F -Ho) T The free energy function for gases may be calculated conveniently by means of statistical mechanical methods when data a~e availa.ble from spectroscopie and electron- diffraction .studies. Third law procedures give the more accurate res.ults since the measurement of the variation in dissociation pressure with temperature is less accurate than the dis~ociation pressure itself. - 30 i To de~ermine bond dissociation energies from equilibrium studies requires a knowledge both of the ' dissociation products and their exact concentration. 1 1 Direct measurement of the total pressure of a gaseous system allows calculation of the partial pressure of, each species on the assum.ption tha.t the gases are ideal. The most precise work of this type was carried out by Perlman and Rollefson (76) on the dissociation equ~librium I 2 ~ 2I, in the temperature range The value D(I2 ) = 35.556 ± 0.023 kcal./ mole thus obtained is in excellent agreement with the 723° to 1274°K. value 35.514 ± 0.050 kcal./mole (77) derived spectroscopically. Indirect methoda of measuring partial pressures generally involve the mea.surement of weight-loss from a system; include the Langmuir and Knudsen techniques. thes~ The Langmuir'technique (78) requires the measurement of the rate of evaporation from a filament of the vaporizing material, assuming there is no activation energy opposing condensation .i The rate of evaporation into a vacuum from unit area of 1a heated surface is given by .!.. 2 aP(M/2~RT) , ' where a is th~ accomodation coefficient, M the molecular weight,, and pl the vapour pressure. 1 For example, this method was applied to the evaluation of the dissociation - 31 energies of the oxides of calcium and strontium (79). The Knudsen method (80) involves the effusion of a gas from a heated cell through a hole of small diameter and infinitely small thickness into an evacuated region. The various, molecular species in the gas phase escape at a rate proportional to their partial pressures. Wise (81) appliep the method to the dissociation of fluorine in the temperature range 500° to 650°K and evaluated D(F 2 ) = 37.6 ± 0.8 kcal./mole from second law considerations. A difficulty in the Knudsen and Langmuir methods is that of unequivocal identification of the vapeur species involved. Inghram, Chupka et al. (82) and Honig (83) solved this problem through development of a mass spectrometer capable of analyzing the high temperature beam. This technique yields heats of vaporization or dissociation from a plot of IT versus 1/T, where I is the intensity of the particular mass signal at T°K, or from third law methods where absolute vapeur pressures can be obtained by comparison of the peak intensity of the substance under study with that for a calibrating substance for which the vapeur pressure is well known. For example, the vapeur in equilibrium with graPhite at 2500°K (82) was shown to consist of C atoms, c2 and molecules, the heats of vaporization of these species i c3 - 32 being 171, 190, and 200 koal./mo1e respectively. An 1 important study of the reaction of graphite with nitrogen at 250d°K by Berkowitz (65) enabled evaluation of the equilibrium constant of the gaseous reaction C + iN ~ CN, and thus, a heat of formation of the 2 cyanide radical of 109 kcal./mole. This is equivalent to D(CN) = 7.5 ± 0.1 ev. and is in agreement with the recent shock wave value of 7. 60 ± 0.13 ev. (84). Goldfinger and Jeunehomme (63) studied the s2 ~. Colin, 2S reaction in,equilibrium with solid calcium sulphide over the temperature range 1750° to 2300°K and derived a value of D(S2) = 97 ± 5 kcal./mole, which supports the spectro- scopie value of 101.5 kcal./mole. The dissociation energies for a series of metallic sulphides were determined by Berkowitz and Marquart (85). Recently, Drowart et al. (86) have derived dissociation energies of the gaseoua monoxides of magnesium, calcium, and strontium and oompared their values with those previoualy obtained using different techniques. To prevent undesirable aide reactions from occurring, the dissociation equilibrium can be established in a flow system so that although a statio concentration of reaotants and produots is set up, the produot molecules do not remain in the reaction zone long enough for aide reactions to occur. - 33 The concentration of the dissociation products is usually determined spectroscopically. Dwyer and Olden- 1 berg (87) s1tudied the equilibrium deduced that D(H-OH) = 118.5 = 100.4 ± 0.9 kcal./mole. 2~0 + 02 ~ 40H and ± 0.7 kcal./mole and D(O-H) The same principles can be applied to flame spectrophotometry in which a solution of a salt of the element studied is sprayed in known concentration into a flame, the temperature of which is measured by the sodium line reversai method. The intensity of a characteristic line of the element is measured and the concentration calculated. The decrease in the concen- tration of the element is assumed to be solely due to the formation of the gaseous diatomic oxide. Uncertainties can result from temperature measurements and the possible 1 formation of gaseous hydroxides. Thus, the dissociation energies represent upper limita. For example, the value D (Mg-0) = 102 kcal./mole, as obtained by Sugden and Bule- wicz (88) from flame spectrophotometry, is about 16 kcal./ mole higher than that obtained by Knudsen maas spectrometry (86). Detonation waves have been used to attain the high temperatures necessary to produce appreciable dissociation in molecules of high stability. 1 A detonation wave is a shock wave maintained by the energy released in a chemical - 34 - reaction. .The wave veloci ty depends on this energy release and therefore on the dissociation equilibrium at high temperatures. K:istiakowsky, Knight and Malin (89) used the measurement of the detonation velocity in the cyanogen-oxygen system to determine the dissociation energies of nitrogen and carbon monoxide. However, only a decision between widely separated values derived by other methods was possible, the most suitable being D(N2 ) = 9.76 ev., D(CO) = 11.11 ev., and D(CN): 7.6 ev. B, Kinet~c Methods Measurements of reaction rates may be used to deduce heats of reaction, since the equilibrium constant is equal to the ratio of the rate constants of the forward and reverse reactions A + B C + D where If the temperature dependance of the rate constants k 1 and k 2 can be expressed by the Arrhenius equation ln k =A - E/RT where E is the activation energy for the reaction, then - 35 the change in internai energy is A knowledge of the temperature dependence of the rate constants allows the calculation of ~E. Kistiakowsky and coworkers (90,91) applied this method to tbe determination of D(CH3-H), using the reactions (1) (2) The occurrence of these reactions in the photobromination of methane was indicated by the measurement of the rate of disappearance of bromine from which the kinetic mechanism was established. The activation energy E was 1 found to be 17.8 kcal./mole, corrections being made for the temperature dependence of the pre-exponential factor. T.he activation energy E2 of the reverse reaction was estimated by analogy to be 1.5 kcal./mole, a value whioh was recently oonfirmed by Fettis and Trotman-Dickenson (92). A E for the reaction between bromine atoms and methane is therefore 16.3 kcal./mole. This value, in oonjunction with the value for D(H-Br), yields D(CH -H) 3 = 103 kcal./mole at 450°K or 101 koal./mole. at 0°K. - 36 Similar studies with various compounds gave bond dissociatio'n energies in agreement with those derived by other methods, with the exception of fluoroform and toluene. A value of 109.5 kcal./mole was obtained by Whittle and' coworkers (93) for D(CF -H), whereas 3 kinetic stuclies of the reaction CF + CH ~ CF H·+ CH 3 4 3 3 indicated a value of 102 kcal./mole. In addition, the 1 heat of formation of the trifluoromethyl radical based on Whittle's studies leads to dissociation energies that are incompatible with the presently.accepted values. For example, the calculated dissociation energies D(CF 3-Br) = 72 and D(CF -F) 3 = 133 kcal./mole are higher than the values of 65 kcal./mole obtained by Sehon and Szwarc (94) from a study of the pyrolysis of CF Br and 3 123 kcal./mole derived by Reed and Snedden (15) from electron impact studies for CF • It is obvious that 4 further investigation is required to clarify these inconsistencies. A value of D(C 6H cH2-H) : 89.5 kcal./mole was 5 obtained from bromination studies, in contrast with the value of 77.5 kcal./mole deduced by Szwarc (74) from pyrolysis studies. Anderson and coworkers (95) found the activation energy for the reaction Br + C6HsCH3 _.,.. C6HsC~ + HBr (1) - 37 - to be 7 kcal./mole and the difference in activation energies for the reactions HBr + c 6H5cH2 Br 2 + c 6H5CH2 to be 5 kcal./mole. --- c 6H5CH3 + Br (2) c 6H5cH2Br + Br (3) As in the analogous reaction in the bromination of methane, the activation energy of reaction (3) was assumed to be zero. change ~ On this basis the energy for reaction (1) was 2 kcal./mole, from which the dissociation energy was calculated. However, as pointed out by Sehon and Szwarc (96) some activation may be associated with reaction (3) which, unlike the analogous reaction with methyl radicals, is only exothermic by about 4 kcal./mole. The derived value of the dissociation energy could therefore be higher by an amount equivalent to E3 and should be considered as an upper limit. The reaction of organic iodides with hydrogen iodide was originally reported by Ogg (97) and subsequently reinterpreted by Sullivan (98) and Benson and 0'Neal (99). From studies of the methyl iodide- hydrogen iodide system, Flowers and Benson (100) determined D(CH3-I), based on the reactions - 38 CH + I 3 2 (1) (2) These reactions were considered to be rate determining steps in the kinetic mechanism as estab1ished from measurements of the rate of formation of iodine. The activation energy for reaction (1) was found to be 20.5 kca1./mole and that of the reverse reaction (2) was estimated to be 0.6 kcal./mole from collision frequencies. This led to a value of 19.9 kca1./mole for the energy change AE, which after correction to 298°K and together with the value for D(I2 ), yielded D(CH3-I) = 55.6 ± 1 kcal. /mole. This agrees favourably with the value 54 ± 1.5 kcal./mole estimated from thermochemical data. Similar studies have yielded bond dissociation energies of 52.0, 53.5, and 40.6 kcal./mole for ethyl iodide (98), trifluoromethyl iodide and benzy1 iodide (101·), respectively. The direct kinetic determination of dissociation energies depends on the assumption that for the unimolecular dissociation reaction the activation energy for the reverse reaction is zero. The activation energy of the forward reaction is then - 39 - equal to the energy change AE of the reaction. In general, dissociation energies based on this assumption are consistent with those derived by other methods. Szwarc (1) derived the expression ku = .KI (1-e -h 'Y0 /kT -D/kT ) e h for the rate constant of a unimolecu1ar reaction in terms of the absolute reaction rate theory. extreme cases were considered: Two (1) h)l0 (( kT, and (2) h>b)) kT, where )10 is the fundamental vibration frequency of the bond. For case (1) which applies to high temperatures or weak bonds, the rate constant reduces to where the experimental activation energy E of the unimo1ecu1ar dissociation reaction is equal to the dissociation energy, D. The pre-exponential factor corresponds with the fundamental vibration frequency of the bond, which is 12 13 -1 about 10 - 10 sec. (77). For case (2) the rate constant becomes ku= U e h -D/kT - 40 where the experimental activation energy E =D t RT and the pre-exponential factor is approximately lol3 sec. -1 at T • 500°K. Thua, this theoretical treatment predicts values of the order of 1012 - 101 3 sec.- 1 for the pre-exponential factors of unimolecular decomposition reactions involving the rupture of one single bond. The direct measurement of the rate of bond fission is often complicated by secondary reactions initiated by the radicals produced in the primary process.. In an ideal system these radicals are removed irreversibly before reaction with the parent molecules occurs. In studies of the pyrolysis of a series of organic iodides, Butler and Polanyi (102) sought to reduce secondary reactions through the use of a flow system in which the reaction time was short and the total decomposition small. A simple reaction mechanism was proposed in which the cleavage of the C-I bond was considered rate determining. R-I __,.... R + I It was assumed that iodine atoms combine to give molecular iodine rather than recombining with radicals, the rate of iodine formation providing a measure of the - 41 initial rate of bond fission. For many iodides, the activation energies calculated with assumed preexponential factors of 101 3 sec.-l yielded bond dissociation energies in approximate agreement with those obtained by other methods (103). However, the mechanism of the pyrolysis is not known with any certainty. Although Szwarc (1) accepted the dissociation energies derived, he criticized the mechanism on grounds that the combination reaction of iodine atoms which is termolecular was not sufficiently fast to prevent the bimolecular back reaction. Alternately, he proposed a chain reaction involving the rapid attack of alkyl radicale on the parent iodide with subsequent decomposition of the iodide radical produced to give an olefin and iodine R + RI R' I - - t.. ~ RH + R' I --1.... olefin + I Benson (104) recently challenged the validity of the basic assumption that cleavage of the C-I bond is the rate determining step and proposed instead two mechanisms considered to be rate limiting in the decomposition of alkyl iodides. - 42 - . RI I + RI HI + olefin ~ I + HI + olefin HYdrogen iodide is maintained at a low stationary state concentration by rapid reaction with the parent iodide to form an alkane and molecular iodine. Whereas such considerations may be valid for a static system, their applicability to a rapid flow system is questionable. Szwarc extended the application of a fast flow system to the pyrolysis of toluene over the temperature range 680- 850°0. At short contact times and low percentage decomposition the experimental data were best explained by the following mechanism. C6H5CH; H + c 6H5cH3 H + C6H5cH 3 1 CH3 + c 6~cH 3 2C6H C~ 5 ~ ____._ .__..... c 6H CH2 + H 5 c 6H5CH2 +~ c 6H6 + CH:? CH4 + c 6H5 C~ ..__.,_ (C6H5CH2)2 The scheme was simplified by the rapid removal of hydrogen atoms and methyl radicals through reaction with - 43 excess toluene and by the thermal stability of the benzyl radical. The initial C-H.bond fission was considered to be rate determining, the speed of the reaction being measured by the rate of formation of hydrogen plus methane. The decomposition was found to be homogeneous and first order with a frequency factor of 2 x 101 3 sec. -l and an activation .energy of 77.5 ± 1.3 kcal./mole which Szwarc identified with 5 D(C 6 H c~-H). However, the accuracy of this value was questioned by Steacie and coworkers (105) who obtained an activation energy of about 90 kcal./molè from similar studies conducted over the higher temperature range 860° to 945°0. In an attempt to explain these discordant values, Takahasi (106) reinvestigated the pyrolysis over a temperature range sufficiently wide to. cover both previous investigations. The plot of log k versus 1/T was found to be slightly curved, the apparent activation energy increasing from about 74 to 104 kcal./mole with increasing temperature. Estimates of the heat of formation of the benzyl radical based on recent thermochemical studies faveur a value of 40 kcal./mole (cf. page 47) which leads to a value of D(C6H5CH2-H) = 80 ± 2 kcal./mole. One of the most successful techniques for the ±2 - 44 determination of bond dissociation energies by kinetic methods is the toluene carrier gas technique developed by Szwarc (1). As evidenced by the thermal decomposi- tion studies, toluene not only possesses a labile hydrogen atom and would provide an efficient radical scavenger, but also forms a thermally stable and unreactive benzyl radical. Szwarc proposed that if a molecule R1R2 were decomposed to form radicale R1 and R2 in the presence of an excess of toluene, these radicale would rapidly abstract a hydrogen atom from toluene to form stable products, and that the benzyl radicale subsequently formed would dimerize to dibenzyl rather than initiate a chain reaction. RlR2 Rl + C6HSCH3 R2 + C6HSCH3 2C 6H5CH 2 ____._ ~·~ R1H + c6H CH2 5 ----.- R H + c H CH2 6 5 2 ----.- (C6ffsCH2)2 ----+- According to this mechanism, the rate of formation of R1R and R2H, which should equal the rate of production of dibenzyl, provides a measure of the initial bond fission. This scheme was applied successfully tà the thermal decomposition of benzyl mercaptan in the presence of an - 45 excess of toluene (70). The decomposition was found to be a first order, homogeneous reaction and the principal products, dibenzyl and hydrogen sulPhide, were formed at equal rates. These observations were explained by the following series of reactions. SH c 61Isc~SH c H CH2 6 5 + C6H5cH3 2C 6H5CH2 c6H5CH2 + H2S + --- SH (C6H5C~)2 The frequency factor was 3 x 101 3 sec.- 1 , and the observed activation energy of 53 ± 2 kcal./mole was identified with the bond dissociation energy. In conjunction with the appropriate heats of formation, this value yields a heat of formation for the hydrosulphide radical of 34.9 ± 4.5 kcal./mole, in agree- ment with the values previously derived from electron impact etudies. Decomposition studies in an excess of toluene are carried out in a flow system with a short contact time 111 tn 1m ri!.e to ·elimilutte possible secondary reactions. The radicals produced should be sufficiently reactive to abstract a hydrogen atom from toluene and be produced at a temperature high enough for this reaction to be rapid. The abstraction reaction is favoured by a high ratio of - 46 - toluene to reactant, preferably greater than 50:1. If the activation energy of the dissociation is to be identified wi th the bond dissociation energy, the decomposition must be established as being a first order unimolecular dissociation reaction. The method is limited to determining dissociation energies that are less than that of toluene, in order to prevent interference from the decomposition of toluene itself. Studies have been made with a large number of compounds including benzyl methyl sulphide (71), benzyl methyl sulpnone (107), benzylamine (108), benzyl bromide (109), ethyl benzene (110), and 1-butene (32). In general, the dissociation energies measured by the toluene carrier technique are in agreement with those derived by other methods within a few kcal./mole. The toluene carrier technique is particularly suited to compounds of the type benzyl-R, where R is a reactive radical, since the large resonance stabilization of the benzyl radical tends to make this the weakest bond in the molecule. However, in ord~r to evaluate the heat of formation of radical R, an accurate value is required for the heat of formation of the benzyl radical. In a review of the thermochemical data available to 1958, Skinner (5) proposed a value of 40 ± 4 kcal./mole ----------'-'----~...._:..,_ __ ................... -·~ - 47 for the heat of formation of the benzyl radical. Two new evaluations which support this proposai can now be made in the light of the recent measurements of the heats of formation of benzyl bromide and iodide by Carson and coworkers (111). A value of 40 ± 2 kcal. /mole is derived from calculations based on the value D(C6H5CH2-Br) = 50.5 kcal./mole (109) as determined by the toluene carrier technique. A similar value of 40.5 ±2 kcal./mole arises from calculations based on the value D(C 6H5CH2-I) = 40.6 kcal./mole (101) as derived from a kinetic study of the reaction Carbop-Su1tihur Bond Dissociation Energies Reyiew Reliable information concerning the bond dissociation energies of sulphur-containing bonds is important for the elucidation of a number of chemical processes. Among these are the vulcanization of rubber (112) and protein transformations (113) such as the permanent setting of hair, the felting and shrinking of wool, and the gelation of egg white and serum albumin. These processes all involve the cleavage or formation of H-S, S-S, or C-S - 48 bonds. Sulphur compounds are being used increasingly in the manufacture of new polymers, such as the polysulphones (114) which are formed by the co-polymerization of olefins with sulphur dioxide. The deter- mination of the kinetic mechanism of this complex polymerization process requires a knowledge of the dissociation energies of the first and second c-s bonds in sulphqnes. Comparatively little information is available on the energy properties of sulphur-containing bonds. The only direct measurements of the dissociation energies of carbon-sulphur bonds are thoae derived either by Franklin and Lumpkin (68) and Palmer and Lessing (69) from electron impact etudies or by Sehon and coworkers (70,71,115) and Busfield and Ivin (107) using the toluene carrier method. In conjunction with other relevant thermochemical data, auch studies yield values for the heats of formation of sulphur-containing free radicale. In a recent review, Mackle (18) selected the following mean values for the radical heats of formation: âllt (SH) : 34 • 6 ± 4 kcal. /mole AHf(SCH3) : 30.5 ± 5 kcal./mole LlHf(SC2~) - 25.5 ± 3 kcal./mole ÂHf (S02CH3) = -60 ± 2 kcal./mole - 49 A series of C-S bond dissociation energies based on these values is reproduced in Table V. Uhless other- wise stated, the uncertainty in the first two columns ±3 is ± 5 kcal./mole and in the last two columns is kcal./mole. The values in pa-r-en +he ses ~Paekets were determined directly. Table Y. Primary c-s Bond Dissociation Energies D(R-SH) D(R-SCH~ (kcal./mole) D(R-SC2~l D(R-S0 2.QR~ CH3 73 72 72 62 (60.5!2) c2~ 71 70 71 64 n-c 3~ 73 72 72 i-C3~ 70 69 70 62 C6H5 78 77 77 48 (49. 5±2. 5) c 6 ~cH2 (53±2) (51. 5±2) 53 - 50 In a study of the thermal decomposition of phenyl methyl sulpnide, Back and Sehon (115) proposed a value of 60 kcal./mole for the dissociation energy, D(C 6H5S-CH3), and concluded that the phenylsulpnide radical was resonance stabilized. It was assumed that the radical resonates between the several canonical structures in a manner analogous to that proposed for the benzyl radical (116). Together with the recently determined heat of formation of pnenyl methyl sulphide (117), this value of the carbon-sulphur dissociation energy yields a heat of formation of 51 kcal./mole for the phenylsulphide radical. However, recent attempts to determine the carbonsulpnur bond dissociation energy of phenyl alkyl sulphides from electron impact studies yielded higher values than that proppsed by Back and Sehon for phenyl methyl s ulphide. Palmer and Lessing (69) found the appearance potential of the phenylsulphide ion from phenyl methyl sulphide to be 12.1 ± 0.1 ev. Combined with the ionization - 51 potential of the phenylsulphide radical, this appearance potential yielded a value of D{C6H5S-CH3) mole. = 83 kcal./ Gowenlock and coworkers (118) derived a similarly high value of D(C6HsS-C 2HS) = 85 kcal./mole based on the appearance potential of the phenylsulphide ion from phenyl ethyl sulphide. This discrepancy was attributed to the formation of a phenylsulphide ion with considerable excess energy. However, an alternate explanation might involve expansion of the parent ion of the phenyl alkyl sulphide to a seven-membered ring before fragmentation, as proposed for the alkylbenzenes (75) and alkyl thiophenes (119). Dinneen and coworkers (120) were able to explain some of the ions produced in the electron impact studies of deuterated phenyl mercaptan by assuming ring expansion in the parent ion. Present Investigation ·The principal aim of the present investigation was to establish the heat of formation of the phentlsulphide radical and to evaluate the carbon-sulphur bond dissocia- tion energies for a series of phenyl organic sulphides. To accomplish this, the thermal decompositions of phenyl ethyl sulphide, phenyl n-propyl sulphide, and phenyl - 52 - benzyl sulphide were studied using the toluene carrier technique. Due to the apparent resonance stabilization of the phenylsulPhide radical, it was expected that the weakest bond in the sulPhides would be the C-S bond joining the alkyl or benzyl radical to the phenylsulphide radical. It was further assumed that the phenylsulphide radical would be formed at a sufficiently high temperature in each of these pyrolyses to react rapidly with toluene to form phenyl mercaptan. In the decomposition of phenyl ethyl sulphide, it was postulated that the ethyl radical produced might not only react with toluene to form ethane, but also decompose to form ethylene plus hydrogen. Regardless of the fate of the ethyl radical, Phenyl mercaptan and c2 hydrocarbons were expected to be formed in equimolar amounts, and consequently, the rate of decomposition could be followed by the rate of production of either product. In the decomposition of Phenyl n-propyl sulPhide, the propyl radical formed was expected to decompose further to yield ethylene plus a methyl radical. If the methyl radicals were to react rapidly with toluene rather than dimerize, then ethylene and Phenyl mercaptan were expected to be formed in equimolar amounts. The rate of formation of either product should, therefore, have given - 53 a measure of the rate of initial bond fission. In the decomposition of phenyl benzyl sulphide, it was expected that the benzyl radicals would dimerize to form dibenzyl rather than recombine with the sulphide radicals. The rate of formation of either phenyl mercaptan or dibenzyl should then have provided a measure of the rate of decomposition. Preliminary resulta of a study designed to determine the sulphur-sulphur bond dissociation energy in diphenyl disulphide are presented in Appendix A. - 54 - EXPERIMENTAL Mate rials P.henyl ethyl sulphide and phenyl benzyl sulphide were kindly supplied by Dr. Hawkins of the Bell Telephone Laboratories, Murray Hill, N.J., and used without further purification. Phenyl n-propyl sulphide was obtained from the Wateree Chemical Co., Lugoff, s.e., by distillation at low pressure. Nitration grade toluene and was purified was supplied by the Gulf Petroleum Co., Pittsburgh, Pa. The toluene was dried and distilled through an efficient column. studies. The fraction boiling at 110.5°0 was used in these Toluene-oG-d 3 was obtained from Merck, Sharp and Dohme, Montreal, P.Q. Appapatus The pyrolysis etudies were conducted in a high vacuum flow system shown in Figure 2. The toluene was introduced into the system from a 100 ml. round-bottom flask, F1 , equipped with a short capillary, c1 • The flask could be maintained at any desired temperature by means of a thermostated water bath, B1 • Weighed amounts of the phenyl etbyl sulphide and phenyl n-propyl sulphide were introduced into the toluene - 55 - stream through a capillar.y tube, c2 , from a detachable vial, F 2 • In the case of the phenyl benzyl sulphide, a weighed pellet of the sulpnide was sealed into a Utube in the toluene flow line. These sections of the apparatus are shown in Figures 3A and 3B, respectively. In both instances, the vapour pressure of the sulpnide was controlled by the heat provided by a removable bath of di-butyl pnthalate, B2 • The flow line leading to the furnace was heated electrically with Nichrome wire to prevent condensation of the sulpnide. A small manometer, M, was connected to this section of the apparatus to measure the flow pressure during an experiment, the pressure being read with a cathetometer to an accuracy of ± 0.001 cm. The reaction vessel, R, shown in Figure 4 was made entirely of silica and was joined to the apparatus with graded silica to pyrex seals. Tlie thermocouple well was sufficiently long to allow measurement of the temperature along the length of the reaction vessel. Section B of the reaction vessel was considered to be the effective reaction volume. The temperature gradient over this section was less than four degrees and dropped sharply across sections A and C, thus minimizing the decomposition in these zones. The temperature in the reaction vessel - 56 was measured by means of a chromel-alumel thermocouple and a Leeds and Northrup potentiometer. The surface dependence of the reaction was examined by using a similar reaction vessel in which section B was packed with quartz woel as supplied by Micro Chemical Specialties, Berkeley, Cal. The average diameter of the fibres used was 3 x lo-3 cm. and the average length 15 cm. The weight per fibre was about 3 x 10-4 g. and about 6.2 g. were used for the packing. The surface area of one fibre was about 0.15 cm. 2 so that the total surface area of the packing was about 3100 cm. 2 The radius of the reaction vessel was 18 mm. and the total surface area about 230 cm. 2 The surface/volume ratio of the unpacked vessel was about 1.1 cm. about 15.1 cm. -1 -1 . and that of the packed vessel The surface/volume ratio was therefore increased by a factor of about 14 in the packed reaction vessel. The reaction vessel was enclosed in a furnace, H, which consisted of a refractory tube (Norton Co., Worcester, Mass.) wound in two sections with Nichrome wire to allow adjustment of the temperature gradient along the reaction vessel. The furnace was thoroughly insulated with rock- woel contained in a metal drum 23 in. in diameter and 2 ft. in length. An Inconel tube was inserted between the - 57 - wall of the refractory tube and the reaction vessel to ensure equalization of temperature. The temperature was regulated by a Thermo Electric controller which maintained the temperature within ± 2°C. The sensing element of the controller was an independant thermocouple inserted in the thermocouple well of the furnace. The exit flow line from the furnace, heated with Nichrome wire, contained a length of capillary tubing, c3 , which controlled the flow rate. This led to a series of three traps, T , T2 , and T . The first trap 1 3 was a removable U-tube of 12 mm. O.D. tubing and the others were of conventional design. The third trap was connected to an analytical section of the apparatus consisting of a gas burette containing a small trap, T4 , and a removable sample flask, F • Non-condensible gases 3 were removed by a high efficiency Edwards diffusion pump, DP, through a small trap, into a series of three bulbs connected by mercury cut-offs. The pressure of non- condensible gases in this collection system was measured by use of a McLeod gauge, MG. A Toepler pump, TP, led to a gas burette that was connected through a mercury eut-off valve to a small trap, T5 , and a copper oxide combustion furnace, CF. - 58 - Figure 2 Apparat us M __~- ..__ TP ' j " 'i ij -~ _ ___..:..___..:..~___..:.._ _ _ _ _ ______;_.......;_____;:_,_;__ __:___ _ _ _ _ _ '1 - 59 - Figure 3A Section of apparatus for the introducti on of liquid sulphides . Figure 3B Section of apparatus for the introducti on of solid sulphides . tToV ~REACTION . TOLU EN E -- ES§ EL __ _ . . i ~ 7~ ~ ~ '--""' . TOLUENE ... _FIG3A TO REACTION t VESSEL . ... PELLET OFSULPHIDE ,. -FIG 38 •. - 60 - Figure 4 Reaction Vessel ___ ........._"·-~--. u·~ !"li/ -<'·tr&,;;,;,?"""Mk' -·'""-·-·-·------ e r e ~ EOGE OF FURNACE 1 . 1 1 THERMOCOUPLE 1 _.. . . . . WELL .. ! ~~T ••: t = '\ ~ t A _ ·/ •; "'\. 8 VOLUME CC LENGTH CM l ------~--·-- 1 "' OUTLET C ? ,. 1 1 1 ·, A 68.5 24.0 . B c 201.5 21.5 20.5 7.5. - 61 The apparatus for gas-liquid chromatograpby was similar ta that described by Ca.llear and Cvetanovic (121) but redesigned ta function as a single pass unit with a reference column. A Gow-Mac thermal conductivity cell, madel TR II B, with tungsten filaments, was used as a detecter. The signal was amplified by a Keithley microvolt-ammeter, madel 150, and recorded by a pen Speedomax Recorder, T,ype G. The power input was regulated with a Sorenson a.c. voltage regulator, madel 500s and a d.c. law power regulator built by the Applied Chemistry Division of the National Research Council of Canada. The apparatus was equipped with sample and reference columns, i in. in diameter and 16 ft. in length, packed with Burrell high activity silica gel. Erocedure and Analyses In the pyrolysis etudies of pnenyl ethyl sulpnide and phenyl n-propyl sulpnide, the samples of sulpnide were weighed and the sample vial attached ta the appara.tus by use of silicone grease on the standard taper joint. In the pyrolysis study of pnenyl benzyl sulphide, weighed pellets of the sulphide were introduced into the inlet U-tube and the inlet arm wa.s sealed. In bath cases the reactant was kept frozen with a dry-ica-acetone bath while - 62 - the apparatus was evacuated to 10 -5 mm. Hg .• pressure. After weighing, the toluene flask was attached to the apparatus through a standard taper joint. It was degassed by successive freezing with liquid air and 5 melting until the final pressure was about 10- mm. Hg. The water bath was adjusted to the desired temperature and placed around the flask. Previous to the start of an experiment, the three product traps, T1 , T , and T , were surrounded with brine 2 3 (-5°C), dry-ice-acetone (-78°C), and liquid air (-l88°C), respectively. Liquid air was also placed around the small trap in the collection system. Immediately prior to the initiation of the toluene flow, the sulpnide sample was warmed to room temperature. The di-butyl phthalate bath was placed around the sample container and the toluene and sulphide were then admitted simultaneously into the reaction system. The toluene flow pressure was generally about one cm., and the partial pressure of sulphide less than one per cent of the toluene flow pressure. The temperature of the bath surrounding the sulpnide was varied from 80° to 100°C with phenyl ethyl sulphide, from 95° to 115°C with phenyl n-propyl sulphide, and from 90° to 115°C with phenyl benzyl sulphide. - 63 The temperature of the reaction vessel and the flow pressure were each recorded at frequent intervals throughout an experiment. ·At the conclusion of the experiment, the toluene flask and the vial of sulPhide were weighed again. In the case of phenyl benzyl sulPhide, the residue remaining after pyrolysis was determined by an amperometric titration (122). In the study of the decomposition of phenyl ethyl sulphide and phenyl n-propyl sulphide, the material collected at -5°C in the first trap, T1 , was weighed and titrated amperometrically for sulphide content with O.lN potassium bromate-bromide solution (122). Dibenzyl was then determined as a difference in weight. A series of experimente were conducted to show that the disulphide content of this trap was negligible. The disulphide was reduced quantitatively with sodium borohydride to mercaptan and the mercaptan was subsequently titrated with O.lN silver nitrate by use of a Radiometer pH Meter equipped with silver and mercurous sulphate electrodes (123). In the pyrolysis of phenyl benzyl sulphide, the disulphide and sulphide content of the material in the first trap were determined in each experiment. The disulphide was reduced to mercaptan by treatment with zinc amalgam according to the procedure outlined by - 64 - Kolthoff et al. (124) and the mercaptan formed was then titrated amperometrically with O.lN silver nitrate solution (125). After precipitation of any excess silver nitrate with hydrochloric acid, the solution was filtered and analyzed for sulphide content. Dibenzyl was estimated as a difference in weight. The second trap, T2, which contained mostly toluene, was removed and the contents were titrated for mercaptan with O.lN silver nitrate solution by use of a rotating platinum electrode and micrometer (125). It was necessary in a series of experimente ta measure the amount of sulphide present in the toluene in arder ta establish a mass balance. This was accomplished by extraction of the mercaptan from a fraction of the toluene with a 10 per cent sodium hydroxide solution to prevent interference in the sulphide titration. The condensible gases trapped at -188°C were initially distilled into the small trap, T4 , that formed part of the gas burette. The product trap, T3 , was maintained at -78°C during the transfer to eliminate any contamination of the products by toluene that may have been carried over from trap T2 • The mercury eut-off valve was closed, trap T4 warmed and the gas measured by a pressure-volume measurement. Fractions of this gas - 65 - were then transferred to the flask, F , for analysis. 3 In the pyrolysis of phenyl ethyl sulPhide, the condensible gases were analyzed for ethane and ethylene content using a gas chromatograPhy column of high activity silica gel. In the pyrolysis of phenyl n-propyl sulphide, the condensible gases were essentially ethylene but contained small quantities of hydrogen sulPhide (about 5 percent of the total). The conden- sible gases were distilled into the flask, F , which 3 contained 10 ml. of lN sodium hydroxide solution kept frozen with liquid air. After warming, the contents of the flask were shaken to promote absorption of the hydrogen sulPhide, acidified and titrated iodometrically (126). The pressure of the non-condensible gases in the calibrated volumes was measured with the McLeod gauge. A sample was transferred by a Toepler pump into the gas burette for combustion over copper oxide at 300oc. The initial pressure of the sample was measured, the sample admitted to the combustion furnace through a mercury eutoff valve and the U-trap, T , surrounded with a dry-ice5 acetone mixture. Within two hours the hydrogen was completely oxidized to water. The residual gas, methane, was returned to the gas burette and the pressure measured. - 66 The composition of the non-condensible gases determined from these measurements agreed favourably with mass spectroscopie results. The decompositions were studied over the temperature range 843° to 935°A for phenyl ethyl sulphide, 832° to 951°A for phenyl n-propyl sulphide, and 759° to 880°A for phenyl benzyl sulphide. - 67 - REiSUL'U? A. AND DISCUSSION Phenyl Ethvl Sulphide Products The main products of the decomposition, as shown in Table VI, were mercaptan, ethane, ethylene, hydrogen, methane and dibenzyl. Mass spectroscopie analysis of the products in the trap maintained at -78°C indicated that the mercaptan was totally pnenyl mercaptan, and that no ethyl mercaptan was present. Large amounts of the undecomposed sulpnide and small quantities of dibenzyl were also identified. The mercaptan, in addition to the undecomposed sulphide, accounted for 99.5 per cent of the sulphide pyrolyzed. Samples of the amperometric titration curves for the mercaptan are shown in Figure 5. Both chemical and mass spectroscopie analyses of the products in the trap maintained at -5°0 indicated only trace quantities of diphenyl disulphide ((2 percent of the mercaptan produced). Similar trace amounts of phenyl benzyl sulphide were detected by mass spectrometr,y. Dibenzyl was identified both by infrared analysis and mass spectroscopie analysis. Dibenzyl and pnenyl ethyl sulpnide accounted for more than - 68 - 97 per cent of the products of this trap. Samples of the amperometric titration curves for sulphide are shawn in Figure 6. The condensible gases were shawn both by gas chromatographie and mass spectroscopie analyses to be exclusively ethane and ethylene. The amount of ethylene varied from 52 to 79 per cent depending on the reaction temperature. A sample chromatogram is shawn in Figure 7. flYdrogen accounted for 65 to 70 per cent of the noncondensible gases, the remainder being methane. The ratio of ethane plus ethylene to mercaptan varied from 0.85 to 1.0. The ratio of hydrogen plus methane to ethylene varied from 0.7 to 1.0, increasing with increasing ratio of toluene to sulphide. The number of dibenzyl radicals produced, considered to be twice the number of moles of dibenzyl formed, was approximately 80 per cent of the total amount of hydrogenated products (methane, hydrogen, ethane and mercaptan). - 69 - Figure 5 Titration curves for mercaptans •• • - . 28 "" Cl) w 0:: w 1 • ... EXPT. 20 1- <( 0 a:: -u ~~ 12 8 1 • 1 • CALIBRATION / 1 • 1. 1 • • 4 1- 1 l. 3.5 .. • 1 . • • 1 1- p. 1 • 0... ~ 16 • 1 2.4 20 1 ' l • 4 . 1 4.5 • 5 VOLUME O.IN SILVER NITRATE SOLUTION (ML.) - 70 - Figure 6 Titration curves for sulphides (. • 14 (J) 12. w a: w ro a_ ~·a o· ' / EXPT. 20 • • ;' l 0:::6 (.) 2.4 2. . / ./ ./ ' _ CALIBRATION • 1 1 . 1 1• j. /• 3 3.5 4.5 4 , VOLUME O.IN BROMATE-BROMIDE SOLUTION (ML) .... ~'--·- ...•. '-"- 'ti"';':·· ......_1 '- 71 - Figure 7 Separation of ethane and ethylene on oolumn of high aotivity silioa gel by gas ohromatograpny. 4~ ,ETHYLENE ~ V) l-l 0 > -_J _J ~ 3~ ........., ETHANE 1- :::r: :x: (!) LLJ 2. .. ::x: <( LJJ a. 1 'u' 17 _,.a 23 ELUTION TIME (MIN,) - 72 - Mechanism of Decomposition The experimental results indicateà that the primary step in the pyrolysis of phenyl ethyl sulphide was the rupture of the C-S bond, (1) with the formation of the phenylsulpnide and ethyl radicals. The phenylsulphide radical reacted with the toluene to form mercaptan, (2) whereas the ethyl radical, in addition to its reaction with the toluene to form ethane, decomposed to give ethylene and a hydrogen atom. c2H5 + c6H5CH3 C2H5 --- c2H6 + c6H CH2 C2H4 + H 5 (3) (4) The decomposition step (4) proposed for the ethyl radical is in accord with the results of Leigh and Szwarc (127) and Bywater and Steacie (128). Previous investigations (74) have shown that hydrogen atoms react rapidly with toluene in this temperature range to give hydrogen and methane. - 73 (5) {6) {7) The dibenzyl formed was considered to have been produced by the combination or the benzyl radicals beyond the 'hot zone' of the reaction vessel. {8) In an attempt to turther elucidate the reaction mechanism, phenyl ethyl sulphide waa pyrolyzed at 627°C in a stream of àeQt&Pate• toluene-oC-d ; isotopie purity or the sample 3 used was 98.8 per cent d3 and 1.2 per cent d2 • The hydrogen and methane produced in the pyrolysis gave the follow1ng isotopie analyses: These resulta indicated that hydrogen atoms and deuterated methyl radicals extracted hydrogen (or deuterium) from both the ring and side chain or toluene-~-d3, action with the side chain being preterred. the re- Similar conclu- sions were reached by Blades and Steacie (129) from a study or - 74 the pyrolysis of toluene-oC-d 3 of low isotopie purity, the major difference being that the extent of deuteration of the hydrogen and methane was less. In addition, an analysis of the benzene produced showed no deuteration, thus indicating reaction (6) to be more important than reaction (9). (9) Cher (130) has shown that at 60°C methyl radicale, derived from the photolysis of azomethane, extract hydrogen with equal probability from the ring or side chain of toluenecC-d3. This result, though surprising, may indicate a difference in the relative reactivities of ring and side chain hydrogena at 60°C and 627°C. The mercaptan produced was found to be only 10 per cent deuterated. This indicated that either the phenyl- sulphide radical reacted preferentially with the ring hydrogena of toluene, or that an extensive exchange reaction occurred between the deuterated thiophenol and the other products in the toluene trap before analysis. An attempt was made to determine the amount of deuteration in the condensible gas products, but contributions of variously deuterated species of ethane and ethylene overlapped to such an extent as to make a confident analysis - 75 - not feasible. The fact that only trace quantities of diphenyl disulphide and phenyl benzyl sulphide were detected indicated that reactions 2C 6H5S c H ssc 6~ (10) c6H5S + c 6 H 5 c~ C6:ffsSCH2c6H5 (11) 6 5 occurred to a negligible extent. The absence of butane in the reaction products showed that the combination reaction (12) did not occur. In a recent review of the reactions of alkyl radicals, Kerr and Trotman-Dickenson (131) have selected a value of kd/kc = 0.14 for the ratio of the rate constants for disproportionation to combination reactions. Since this ratio appears to be temperature independant, then reaction (13) may also be negligible. (13) The proposed mechanism for the pyrolysis of phenyl ethyl sulphide requires that: (a) one mole of c2 hydrocarbons be produced for every mole of phenyl mercaptan, - 76 - (b) one mole of hydrogen be produced for each mole of ethylene, (c) one-half a mole of dibenzyl be produced for each mole of phenyl mercaptan or c2 hydrocarbons. The experimental evidence seems to support these conclusions. The fact that the amount of c2 hydrocarbons is generally slightly less than the amount of phenyl mercaptan produced may indicate that some of the ethyl radicals were removed by combination with benzyl radicals rather than by reaction with toluene. The extent to which dibenzyl is formed supports the conclusion that the decomposition of phenyl ethyl sulphide occurs via a radical split. This eliminates the possibility of an intramolecular rearrangement. (14) The first order rate constants for the decomposition of phenyl ethyl sulphide were calculated from the rate of formation of thiophenol, and are recorded in Table VI. sample calculation is shown in Appendix B. A The effect of changes in the contact time, partial pressures of phenyl ethyl sulphide and toluene are shown in Tables V.II, VIII, and IX, respectively. The effect of the increased surface/ volume ratio in the packed reaction vessel is recorded in - 77 - Table X. T.hese resulta suggest that the decomposition is a first order homogeneous process. As observed in Table VIII, the k values increased slightly with increasing toluene pressure. This may indicate that radical recombination reactions occurred to a minor extent at lower toluene pressures. However, it was not experimentally feasible to operate at the higher pressures necessary to obtain sufficient data to make an extrapolation of k values to infinite pressure. The plot of log k versus 1/T is given in Figure 8, the straight line corresponding to an activation energy of 59.5 kcal./mole and a frequency factor of 6 x 1014 sec.- 1 The temperature dependance of the ratio of ethane to ethylene can be expressed approximately by the equation as shown in Table XI. Based on the rate equations for reactions (3) and (4), the ratio of ethane to ethylene should be = - 78 If 4 E ~40 kcal./mole as suggested by several workers (128,132), then E is about 13 kcal./mole. 3 The activation energy for hydrogen abstraction reactions involving ethyl radicals could be as much as 4 kcal./ mole higher than for those involving methyl radicals, since D(C 2Bs-H) is about 4 kcal./mole less than D(CH -H). 3 In view of this fact, the calculated value of 13 kcal./ mole is compatible with E15 = 8.3 kcal./mole as determined by Trotman-Dickenson and Steacie (133) for the reaction - (15) and gives further support for the proposed mechanism. Bond Energies From the experimental results the activation energy of the initial dissociation process (1) was derived as 59.5 kcal./mole. If the recombination of the phenylsulphide and ethyl radioals is assumed to take place without any activation energy, as is usual for the recombination of free radicals, then D(C 6H5s-c 2H ) may be 5 identified as 59.5 kcal./mole, with a probable error of ! 2 kcal./mole. - 79 This is considerably lower than the value of 85 kcal./mole implicit in the electron impact studies of Gowenlock and coworkers (118). However, these authors considered that the higher value might be due to a rearrangement process, rather than to dissociation of the c-s bond. From the equation in conjunction with the recently determined value of ~Hf (C6H 5sc2H5) = 18.4 :t 0.7 kcal./mole (117) and the ) = 25.5 ± 2 kcal./mole (5), i t follows 5 that the heat of formation of the phenylsulphide radical, value of ~Hf (C 2H 6Hf(C6H5S), is 52.4 :t 4.7 kcal./mole. This compares favourably wi th the value of 6Hf (C H S) = 51.0 ± 3. 7 6 5 kcal./mole calculated from the values D(C6H5S-CH ) = 60 3 ±2 kcal./mole, as determined by Back and Sehon (115), and 6Hf(C6H5ScH3 ) = 23.5 ± 0.7 kcal./mole (117). Based on the value D(C 6H5CH2 -scH 3 ) = 51.5 kcal./mole, as determined by Braye, Sehon and Darwent (71), Mackle (18) proposed a value of 30.5 ± 5 kcal./mole for Together wi th the appropria te values for 6Hf (C 2H5 ) and ô. Hf CCH3SC2H5 ) (134), this value yielded D (CH 3s-c 2H ) = 5 70 ±5 kcal./mole (as shown in Table V). 3 ~Hf(SCH ). - 80 - The difference would therefore represent the difference between the resonance energies of the methyl sulpnide and phenylsulphide radicals. Renee, the experimental resonance energy of the phenylsulphide radical, Re(C 6H5S), is probably equal or larger than 10.5 kcal./mole. This compares favourably with the value of 12.0 kcal./mole proposed by Back and Sehon. - 81 - Figure 8 Plot of log k vs. 1/T Filled circles denote experiments done in packed vessel. ------------------~-·-·--~---···· .8 .6 .4 . .z 1.09 1.10 1.12 1.14 1/T X 103 1.16 f.f8 - 82 - Table VI Products of the decomposition of phenyl ethyl sulPhide e e i'1l <1> i'1l i'1l Cl> +> Pi < 0 0 Cl> i'1l F-I p.;M r-1 os M~ E-1 31 843 •726 11.74 33 843 •715 21 853 30 r-1 0 t ~ r-1 :;:$ i'1l "Bm 0 omCl> i'1l ~ ~ Pi'll 0~ i'1l <1> Cl> ~..;t 0 ~i'll Cl> 'Or-1 PO oa os ~ \0 ~ C\1 ~ ~..;t ~T r-1 0 r-1 m Ni'll P<l> Cl> r-i ,00 :>:. Cf.) a AS ~ rS( 1 r Pi ,0+ • ..;t f=l~ 0 !><+ (\J ~~~..;t ~r~ a 0 0 <1> A r-1 1 0 Cl> i'1l f:i!'it!:l C\1 ~ 130 .092 65.7 34.3 .160 46.2 53.8 .204 .116 .79 .63 1.07 13.0 .190 11.56 384 .056 63.7 36.3 .066 47.2 52.8 .112 .164 .59 1.65 1.62 13.4 .196 .243 11.84 133 .101 64.0 36.0 .140 40.5 59.5 .194 - 1.21 6.5 .272 853 •726 11.65 102 .176 67.9 32.1 .340 39.3 60.7 .410 38 857 .604 17.84 253 .133 64.1 35.9 .215 48.8 51.2 41 857 .587 6.47 75 .112 70.2 29.8 .245 34.3 20 863 .238 11.75 131 .178 66.6 33.4 .299 29 863 .728 11.51 85 .187 68.5 31.5 34 863 .715 11.60 221 .092 67 .o 44P 863 .245 11.25 135 .140 37 867 .588 17.88 285 42 867 .600 6.48 13 871 .254 10.56 +> e-ca Cf.) 0 C\1 0 ~ ·r-i C\1 C\1~ li1 ,.!4 . 72 - .211 .83 .59 .85 18.4 .276 .260 .152 .83 .61 1.21 18.4 .335 65.7 .285 .220 .86 .92 .70 15.0 .286 35.8 64.2 .343 .252 .87 .80 .93 9.3 .415 .388 40.0 60.0 .457 .352 .85 .88 .81 25.7 .405 33.0 .143 34.7 65.3 .186 .129 . 79 •79 .99 27.9 .456 65.7 34.3 .267 28.8 71.2 .300 .292 .89 1.13 .74 10.5 .430 .148 64.5 35.5 .250 32.9 67.1 .290 .264 .86 1.01 .88 27.9 .555 110 .104 - - .145 32.5 67.5 .205 .162 •71 .91 1.06 26.1 .503 228 .160 66.0 34 .o .259 28.6 71.4 .300 .200 .87 •75 .90 15.1 .653 e e 1 III tf.) r-1 Dl Q) m m Q) ex: +' 0 Pl ~0 r=<:~l2i E-1 0 Q) Dl +' H ~~ r-1 os E-IS r •r-I ,.g Pl r-1 r-1 0 roS J:l 0 s oroQ) J:lOl oro Dl Dl Q) Q) Dl ~ ~ ro t!:lm III"<T ror-1 J:lO 12it!:l III 0 91 .095 80.0 20.0 C\1 ~ Q) os os .187 :;:::$ tf.) ~ \.0 III III"<t- 0 0 C\1 C\1 r-1 0 ~ 1 III tf.) r-1 t>;, NOl J:l Q) <l>r-1 ,.co ·r-1 a ~ l \.0 t::JIII J:lC\1 <DO ,b + ·r-I 1=1 IIIItn + ~ 0 ~+ Pl C\1 IIII"<T +III s0 0 Q) 1=1 r-1 1 0 Q) Dl ~~ ~ .81 . 70 15.4 •705 .94 - •70 16.4 .657 1.05 - - 16.7 .675 .89 .72 1.01 ocr' .140 .94 I=IS C\1 C\1 III .!<l 10 873 . 705 10.61 11 873 .280 12.90 94 .167 67.8 33.2 .342 30.0 70.0 .366 2 875 .273 11.50 182 .124 84.7 15.3 .515 - - .490 19 883 .240 10.93 176 .197 67.7 32.3 .314 38.0 62.0 .355 25 883 .246 5.56 96 .163 76.2 23.8 .352 25.3 74.7 .383 - .92 - .62 21.9 .990 28 883 . 730 11.50 125 .167 70.0 30.0 .338 34.0 66.0 .392 .288 .86 .86 . 75 50.0 .945 45P 883 .241 11.55 150 .173 66.0 34.0 .302 26.9 73.1 .325 .230 .93 . 79 .80 20.3 .950 36 889 .580 16.78 384 .148 62.5 37.5 .243 33.0 67 .o .275 .223 .88 .89 .91 57.8 1.47 14 892 .242 11.61 410 .167 65.7 34.3 .246 29.5 70.5 .285 .86 - .97 30.5 1.51 22 892 .243 11.06 122 .264 73.3 26.7 .509 27.0 73.0 .550 .340 .93 . 72 •71 26.7 1.39 35 898 .698 11.19 168 .180 69.9 30.1 .320 32.6 67.4 .365 .313 .88 .97 .81 73.0 1.88 18 899 .247 10.90 194 .187 71.8 28.2 .305 25.6 74.4 .350 .247 .87 .80 .83 37.0 1.87 27 904 .693 11.01 .181 67.4 32.6 .234 23.5 76.5 .374 .204 •79 .67 1.01 79.2 2.25 510 27.5 72.5 .200 .240 - 21.5 1.01 e e tf.l (1) tf.l tf.l (1) < +> 0 A MO J":i!IZi 8 0 (1) tf.l +> ~ P-1~ r-1 os E-iS r ! :;:$ r-1 0 ros §S Otf.l (1) !=ltf.l Oct! tf.l tf.l tf.l r-1 (1) ~ C\1 ~ -.:;jIJ:1 ~tf.l(1) ror-1 !=lO os (1) ~ \.0 IJ:1 C\1 ~ p:j-.:;jC\1 0 ~ r-1 p:jr ~ C'lJ Ntf.l j:lCD CD r-I 1 ,co ro I=IS IJ:1 •rf s ~1 IJ:1Iro o<)' r· • Pt s0 -.:;j- f=~p:j :${p:j-.::r 0 C\1~ i~ 1=1 0 + (1) r-1 1 0 (1) tf.l 0 oa 0 72.8 27.2 .274 22.2 77.8 .324 .220 .85 •79 .82 48.5 2.13 ro Jzit!l IJ:1 250 .177 0 ~ .!.4 24 904 .310 6.10 26 904 .227 11.66 480 .264 67.3 32.7 .441 21.7 79.3 .482 .320 .92 •76 •76 40.0 2.23 46P 904 .235 11.64 235 .177 69.2 30.8 .288 25.0 75.0 .310 .226 .93 .81 .82 40.5 2.20 17 911 .240 11.28 395 .314 70.2 29.8 .486 21.0 79.0 .550 .4(]7 .88 .84 .82 51.8 3.04 23 915 .233 10.96 345 .187 68.5 31.5 .279 22.5 77.5 .330 .247 .85 .85 .87 55.8 3.50 8 916 .277 13.21 165 .118 95.3 4.7 .615 20.9 79.1 .625 .431 .98 .99 .24 57.0 3.03 16 923 .234 11.44 225 .300 73.2 26.8 .488 22.5 77.5 .550 .362 .89 •76 .80 68.0 4.85 47P 923 .228 11.35 316 .186 70.0 30.0 .270 20.7 79.3 .290 - .93 - .87 66.0 4.72 15 .315 11.62 242 .315 71.8 28.2 .510 20.4 79.6 •565 .90 .99 •78 79.1 6.85 935 .490 - 83 Table VII Tqe Decomposition of P.henyl Ethy1 Su1tihide variation of k with Contact Time Expt. No. T oA Contact Time k sec. sec.- 1 21 853 0.243 0.272 30 853 0.726 0.276 20 863 0.238 0.415 29 863 0.728 0.405 11 873 0.280 0.657 10 873 o. 705 o. 705 19 883 0.240 1.01 28 883 0.730 0.945 18 899 0.247 1.87 35 898 0.698 1.88 26 904 0.227 2.23 27 904 0.693 2.25 - 84 - l'able VIII The Decomposition of P.henyl Ethyl Sulpnide Variation of k nith the Partial Pressure of Sulpnide Expt. No. T OA Sulphide Pressure k mm. sec.-1 Hg 31 843 0.090 0.190 33 843 0.030 0.196 29 863 0.135 0.405 34 863 0.052 0.456 11 873 0.137 0.657 2 875 0.063 0.675 22 892 0.091 1.39 14 892 0.028 1.51 8 916 0.080 3.03 23 915 0.032 3.50 - 85 - Table IX The Decomposition of Phenyl Ew;yl Sulpnide variation of k with Toluene Pre§ sure Expt. No. T OA Toluene Pressure k mm. sec. -1 Hg. 38 857 17.84 0.335 41 857 6.47 0.286 37 867 17.88 0.555 42 867 6.48 0.503 19 883 10.93 1.01 25 883 5.56 0.990 26 904 11.66 2.23 24 904 6.10 2.13 - 86 Table X ~e Decompositio n of P.henyl Ethyl Su1tihide Effect Qf the Packed Reaction Vesse1 on k Expt. No. T k OA sec.- 1 20 863 0.415 44P 863 0.430 19 883 1.01 45P 883 0.95 26 904 2.23 46P 904 2.20 16 923 4.85 47P 923 4.72 - 87 Table XI A Comparison of Abstraction and Decompos1tion Re~ctions C 2 H~ C2H4 Expt. No. fgr c2E5 : 3.5 x 10-4 e27000/RT(C6H5CH3) T Toluene OA moles_ litre 1 e27000/RT C2H6 C2H4 Cale. Exper. 2.24 x 10- 4 2.20 x 10- 4 11.2 x 106 11.2 x 106 0.87 0.86 0.86 0.89 2.23 x 10-4 2.21 x lo- 4 8.9 x 10 6 8.9 x 10 6 0.69 0.68 0.68 0.65 2.19 x 10-4 2.16 x 10- 4 7.4 x 106 0.57 0.56 7.4 x 106 0.56 0.53 6.4 x 106 6.0 x 10 6 0.44 0.40 873 1.95 x 10-4 1.95 x 10- 4 0.41 0.38 11 873 2.38 x 10- 4 0.50 0.43 28 883 0.39 0.51 14 892 2.10 x 10-4 2.09 x 10- 4 6.0 x 106 5.2 x 10 6 0.33 0.42 22 892 4.5 :x: 106 4.5 x 10 6 0.31· 0.37 18 899 0.27 0.34 27 904 4.0 x 106 3.8 x 10 6 0.26 0.31 26 904 0.28 0.27 17 911 0.22 0.27 23 915 1.99 x 10- 4 1.92 x 10- 4 3.8 x 106 3.1 x 10 6 0.21 0.29 16 923 2.00 x 10- 4 3.1 x 10 6 2.7 x 10 6 0.19 0.29 15 935 1.95 x 1o-4 2.2 x 106 0.15 0.25 31 843 33 843 21 853 30 853 20 863 34 863 13 871 10 1.99 x 10- 4 1.95 :x: 10- 4 1.95 x 10- 4 2.07 :x: 10- 4 - 88 - B. Phenyl n-Pronvl Sulnhide Products The main products of the decomposition, as shawn in Table XII, were mercaptan, ethylene, methane and dibenzyl. Bath chemical and mass spectroscopie analyses of the products collected in the trap maintained at -5°C indicated only trace quantities of diphenyl disulpnide (less than 2 percent of the mercaptan produced). The sulphide content was predominantly phenyl n-propyl sulphide, although minor amounts of phenyl benzyl sulphide (about 7 per cent) and pnenyl methyl sulpnide (about one percent) were detected. Dibenzyl and phenyl n-propyl sulphide accounted for more than 96 per cent of the products of this trap. Mass spectroscopie analysis of the products collected in the trap maintained at -78°C indicated that phenyl mercaptan and phenyl n-propyl sulphide were the major constituants. No propyl mercaptan was present although small quantities of phenyl methyl sulphide and dibenzyl were detected. The mercaptan, in addition to the sulphides present in the two initial traps, accounted for 98 percent of the sulphide pyrolyzed. The condensible gases were essentially ethylene, the principal impurities being propylene (about 2 per cent) - 89 and hydrogen sulphide (about 4 percent). The former was detected by mass spectrometry and the latter, which was initially detected both by mass spectrometrie and gas chromatographie analyses, was subsequently determined iodometrically. Trace amounts of ethane were also observed. Methane accounted for more than 95 per cent of the non-condensible gases, the remainder being hydrogen. In general, the hydrogen was considered sufficiently small to be neglected. Both the ratio of mercaptan to ethylene, which varied from 0.7 to 1.0, and the ratio of methane to ethylene, which varied from 0.6 to 0.9, ratios of toluene to sulphide. increas~~ with the increasing sum~+he TheVnumber of moles of mercaptan and methane formed is approximately twice the number of moles of dibenzyl. Meçhanism of Decomposition The experimental results indicated that the primary step in the pyrolysis of phenyl n-propyl sulphide was the rupture of the c-s bond, (1) - 90 - with the formation of the phenylsulpnide and n-propyl radicals. The phenylsulphide radical reacted with the toluene to form mercaptan, (2) whereas the n-propyl radical decomposed to give ethylene and a methyl radical (3) The small amounts of hydrogen and propylene formed indicated that a second mode of decomposition of the n-propyl radical occurred to a minor extent (4) These modes of decomposition of the n-propyl radical are in accord with the studies of Eywater and Steacie (135) and Kerr and Trotman-Dickenson (136). The reaction was more complex since the methyl radicals did not react completely with toluene to form methane. ... (5) Szwarc and Taylor (137) have shown that at 780°C about 25 per cent of the methyl radicals produced in the thermal decomposition of acetone were removed by combination with benzyl radicals - 91 - CH:3 + c 6rr crr2 5 .__..... c 6rr5crr2cH 3 (6) and about 1 to 2 per cent by dimerization CH3 + CH (7) C2H6 3 The presence of pheny1 methyl su1phide in the products of the trap maintained at -78°0 indicated that some of the methy1 radica1s were a1so removed by combination with pheny1su1phide radicals (8) A pyrolysis of pheny1 n-propyl sulphide at 900°K in a stream of toluene-~-d 3 produced methane of the fo1lowing isotopie analysis: Thus the attack of the metbyl radical was directed both to the side chain and ring hydrogens, the former being more reactive. Similar conclusions were reached for the reaction of deuterated methyl radicals on toluene-oe-a 3 in the pyrolysis of pheny1 ethyl sulphide. Since on1y trace amounts of diphenyl disulphide and phenyl benzyl sulphide were detected, it may be concluded that reactions _______ ......... ------~---------------.....:......__ -~· -~-·· - 92 - .... (9) (10) occurred only to a negligible extent. The minor amounts of hydrogen sulpnide were apparently produced in a side reaction, the exact nature of which is open to speculation. Since D(C 6H -SR) where 5 R = H, CH3, c2H5 , has a value of about 77 kcal./mole (see Table V), it appeared improbable that hydrosulphide or alkyl sulphide radicals could be produced in significant amounts as intermediates, from which hydrogen sulphide could be derived. However, it may be possible that an isomerization similar to that occurring in the +k ta.«.lka.nes linear tftielkaEea (138) takes place in the phenyl n-propyl sulphide to form benzyl ethyl sulphide. Such an isomer would readily decompose under the conditions of this pyrolysis to give ethylsulphide radicals, a source of hydrosulphide radicals. (11) (12) (13) (14) - 93 Based on reactions (1) to (10), the simple mechanism proposed for the pyrolysis of pnenyl n-propyl sulpnide requires that: (a) one mole of mercaptan be produced for each mole of ethylene, (b) one mole of methane be produced for each mole of ethylene, (c) one-half a mole of dibenzyl be produced for each mole of methane and mercaptan. In general, the experimental results support these conclusions. Deviations of the ratios from unity can be attributed to side reactions of the methyl radicals to form pnenyl me thyl sulpnide and ethylbenzene. '!he amount of dibenzyl measured together with the knowledge that some dibenzyl has been lost due to inefficient trapping indicates that the primary mode of decomposition of pnenyl n-propyl sulpnide occurred via a free radical process and did not involve an intramolecular rearrangement such as reaction (15). .. (15) The first order rate constants for the decomposition of pnenyl n-propyl sulpnide were calculated from the formation of ethylene and are recorded in Table XII. - 94 The effect of changes in the contact time, partial pressures of phenyl n-propyl sulphide and toluene are shown in Tables XIII, XIV, and XV, respectively. The effect of the packed reaction vessel on the first order rate constant is indicated in Table XVI. These results are compatible with a first order homogeneous reaction. The plot of log k versus 1/T, given in Figure 9, is remarkably linear, thus indicating the validity of this treatment of the experimental data. The straight line corresponds to an activation energy of 60.0 kcal./ mole and a frequency factor of 8 x 1014 sec.-l Bond Energies The experimental results indicate that the activation energy of the initial dissociation process is 60.0 ~cal./mole. If the recombination of the phenyl- sulphide and n-propyl radicals occurs without any H?) activation energy, then D(C6H5s-n-c 3 is equal to 60.0 kcal./mole, with a probable error of± 2 kcal./mole. The equation - 95 can be employed to calculate the heat of formation of the phenylsulpnide radical. Although the heat of formation of pnenyl n-propyl sulphide has not been determined, it can be calculated from the known value of b.Hf(c 6H5sc 2H5 ) = 18.4 kcal./mole (117) by use of Franklin's group method (139). 5 b.Hf(C 6 H S-C3~) - .6.Hf(C 6H sc 2H ) + .6.Hf(-CH2 -) 5 5 = 18.4 - 4.9 = 13.5 kcal./mole In order to calculate the heat of formation of .... the phenylsulphide radical, a reliable value is required for the heat of formation of the n-propyl radical. Skinner (5) ini tially proposed a value of ÂHf (n-c 3~) 22 ± 3 kcal./mole based on the electron impact deter- minations of Stevenson (140). However, Calvert and Sleppy (141) and Kerr and Calvert (142) recently found 34.9 and 34.5 kcal./mole as the activation energy for the decomposition of the propyl radical. In combination with Brinton's (143) activation energy for the addition of a methyl radical to ethylene, these values yield D(n-c 3H?-H) = 97.3 kcal./mole. In the light of this, Pope and Skinner (144) have proposed a new value of ÂHf(n-c 3H7 ) = 20.5 ± 2 kcal./mole which, in conjunction with ÂHf(C6H5S-C3H?) = 13.5 ~ 1 kcal./mole, gives the heat of - 96 - formation of the phenylsulphide radical as - 53.0 ~ ~Hf(C H S) 6 5 5 kcal./mole. This value agrees, within experimental error, with the previously determined values of 51 kcal./mole from the pyrolysis of phenyl methyl sulphide and 52.4 kcal./ mole from the pyrolysis of phenyl ethyl sulphide. As recorded in Table V, Mackle (18) calculated D(n-c 3H?-SCH 3 ) - 72 ± 5 kcal./mole, based on the value 3H7 ) = 22 ± 3 kcal./mole. However, the actual dissociation energy should be 1.5 kcal./mole lower in ~Hf (n-c view of the more recent value of ~Hf (n-C H7 ) 3 kcal./mole. = 20.5 ± 2 The difference may then be considered to represent the difference between the resonance energies of the methyl sulphide and phenylsulphide radicals, which may be identified as a lower limit for the resonance energy associated with the phenylsulphide radical This value is identical to that obtained in the pyrolysis of phenyl ethyl sulphide and 1.5 kcal./mole lower than - 97 that obtained in the pyrolysis of phenyl methyl sulphide. The consistency of the values for both ÀHf(c H S) 6 5 and Re(C H S) further supports the validity of the 6 5 conclusions derived in these studies. - 98 - Figure .9. Plot of log k vs. 1/T Filled circles denote experimenta done in packed vessel. 1.0 .a .6 .4 .2 ~0 (.!) 0 ..J-.2 -.4 -.6 -.a 0 1.06 1.08 1.14 1.12 1.10 1/T X 10 3 . l · .. ''·:.·'1 . :,_:.;i '·. ·. ~ ·, ..· ' .. ' 1.16 1.18 1.20 - 99 - Table XII Products of the decomposition of Phenyl n-propyl sulPhide - e (!} M~ ..j...) Pl o < 0 8 ~ ~ 8~ 0 <D Q) ~ p., _tlO (!} IJ:l (1) ~ ·r-i .d ·p. (!} a> r-l o:::ta ~ (!} œ t!:s ~ <D r-l o Jro 11:1 om 12.24 lOO .209 .232 r-l o r-l r-l ::1 J:! o a oa § +-> ~ ~ ~a o:::t 11:1 rn 0 IJ:l C\1 . Ç\1 Pl r-l >., (!} t'J (!} 0 r-l ~ o <D Q) .0 r-l «1 a> a J:~ <D ·r-i o a RS ~0 ~ 1 o:::t o:::t C\1 C\1 11:1 ~ 11:1• rn + .:f ....... 0 a r-l r ~ ~ Pl 0 o 0 <D Q) (!} 1=1 .230 .195 1.01 .85 .89 10.8 .112 0 .250 .204 .95 .80 .86 15.5 .175 3.7 .280 .248 -73 .60 .97 17.8 .205 0 .165 .110 1.14 1.07 .69 17.2 .226 95.2 4.8 .173 .127 .87 .75 .79 5.9 .237 .300 95.0 5.0 .265 .207 -93 .75 .85 22.4 .262 .351 .491 97.4 2.6 .430 .362 .go .74 .93 22.0 .326 63 .218 .406 98.1 1.9 .302 .190 .76 .55 .73 27.9 .310 139 .123 .168 94.1 5.9 .150 .95 .78 - 19.9 .303 .925 12.63 183 .209 .248 99.0 1.0 .255 .103 1.04 .85 .45 31.0 .423 859 .262 10.15 130 .183 .275 96.4 3.6 .215 .204 .81 .69 1.02 11.0 .440 66P 859 .248 10.39 147 .136 .182 97.3 2.7 .150 .105 .85 .77 .73 8.9 .400 20 868 .289 12.91 108 .245 .444 94.4 5.6 .320 .182 .76 .58 .64 17.4 .669 1.01 35 832 36 839 .975 12.17 120 .210 .264 37 839 .944 12.12 43 .231 .399 33 846 .955 12.39 317 .155 .145 49 847 .252 10.70 136 .148 .209 34 848 .965 12.39 130 .214 42 854 .746 20.37 15s 43 854 5.72 44 855 .730 5.24 32 859 47 1.05 99.0 1.0 lOO 96.3 lOO - e tl m m Q) c::t: +> 0 Pl ~0 0 Q) m H P-t~ r-1 ~~ li m Q) m m ~m Q) r-1 Q) 'Or-1 os g~ 39 .264 .623 fl:l~ Ho ri:!~ E-1 +> 21 870 .295 12.63 22 870 .298 11.48 448 .085 .110 23 875 •740 20.78 160 .240 .350 24 875 11.76 91 .266 .523 38 880 .926 12.28 281 .238 .300 60 883 .294 5.70 76 .148 .334 65P 883 .240 10.77 189 .131 7 883 .273 12.55 185 31 883 .935 12.33 41 891 .705 18 894 29 30 H ai ....., fl:l~ ca(\J (\J 0 fJ:l ~ ~ 96.8 P!m «JQ) Or-1 HO a>S ::l!EiS NI H Q) r-1 ~ ,.0 •ri ts~m HCI.> Q)r-1 Pl IJ:I + R ca s0 0 Q) r-1 1 0 Q) m s ·~:: .220 .50 .44 .78 19.4 .718 .89 .77 - 18.8 .702 ,.00 •ri AS ~ fl:l~ ~~ J4 ~ 0 0 (\J R ~ ,!4 3.2 .300 0 .098 97.1 2.9 .285 .150 .84 •71 .57 44.8 .802 96.6 3.4 .350 .220 .69 .53 •72 57.6 .809 0 .295 .220 .98 •79 .82 56.2 .882 94.0 6.0 .200 .200 .64 .47 1.15 27.9 1.13 .186 96.8 3.2 .146 .110 .81 •73 .80 21.8 1.04 .201 .340 94.1 5.9 .250 •78 .63 - 27.0 1.14 170 .238 .357 98.0 2.0 .311 .220 .89 .68 .80 67.4 1.19 19.75 615 .300 .403 97.5 2.5 .374 .275 .95 •76 .82 63.6 1.46 .276 12.72 180 .320 .514 99.0 1.0 .425 .230 .84 .63 .60 40.0 1.84 894 .900 12.50 130 .247 .435 90.8 9.2 .324 .200 .82 .63 .70 74.0 1.50 895 .912 12.60 382 .165 .190 97.4 2.6 .190 .200 1.03 .89 1.13 72.5 1.49 1.04 100 100 - - e e fJ2 fJ2 fJ2 Q) < +> 0 A 0 Q) fJ2 H P-i~ rl Q) r •r-I fJ2 fJ2 ~ rorl P=l ~ 0 os os 81 .354 .850 .490 1.22 ii rl '<:;J-0 Ml2:i E-1 +> os E-fS 19 897 .269 12.90 28 897 .890 12.60 13 39 902 .894 12.31 205 .376 58 902 .226 10.65 235 59 902 .292 5.76 63P 902 .239 53 906 6 ~0 ct! tbro ::$ tf..! Q) PO tf..! C\1 (\( Aro NIZl P<l> ctl<l> Orl Q) p.. <Drl '<:;j- A tf..! 0 + Q) rl 1 0 Q) m ~~~(\( .225 .57 .43 .55 42.5 2.03 .46 .42 - 83.5 2.03 HO .00 ~ ~a AS <I>S a0 P=l '<:;j- A 1 .a •r-I a P=l 0 ~ rl +> tt N l=l ~ .,-~ ~~ 0~ (\( 0 p::'<:;j- A ~ ..!:4 97.1 2.9 .470 95.7 4.3 .540 .570 98.3 1.7 .510 .354 .91 .67 .80 84.5 2.07 .186 .328 94.5 5.5 .250 .192 .81 .60 .88 39.1 2 .·18 122 .177 .285 96.5 3.5 .240 .209 .87 .65 1.00 47.0 2.17 10.85 276 .158 .187 0 .176 - .94 .85 - .374 11.35 204 .252 .435 92.0 8.0 .335 .260 .84 .63 .89 913 .222 12.47 440 .197 .325 96.5 3.5 .248 .222 •79 .63 1.00 56.2 3.75 50 913 .231 9.57 160 .240 .451 96.7 3.3 .335 .318 .77 .55 1.10 53.9 3.36 1 913 .260 11.71 200 .290 .450 0 .390 .280 .87 • 65 .82 60.0 3.52 52 915 .368 13.25 830 .173 .228 96.5 3.5 .204 .93 •79 - 69.8 3.47 14 927 .267 12.00 230 .400 .718 96.5 3.5 .565 .395 .82 .58 .82 77.1 5.50 15 927 .242 12.00 .288 .736 95.1 4.9 .400 .234 .57 .41 .68 76.0 5.87 42 lOO 100 - - 42.3 2.29 62.0 2.60 - r-1 m m ~..;t r-1 ror-1 C\l 56 927 .082 8.32 165 .177 .311 95.2 4.8 .220 - .74 .60 61 927 .295 5.84 156 .201 .400 97.5 2.5 .306 .209 •79 .54 .82 78.0 5.14 62 927 .221 11.16 307 .248 .426 95.3 4.7 .345 .236 .85 .61 .80 72.3 5.75 64P 927 .226 10.66 252 .189 .288 95.5 4.5 .250 .184 .91 .69 .84 75.4 5.67 11 935 .265 12.16 83 .290 .610 96.8 3.2 .420 .255 .69 .48 •72 89.0 7.45 55 941 .087 7.53 488 .161 .323 93.8 6.2 .220 .170 •73 .53 . 90 50.8 12 951 .276 12.25 159 .236 .464 95.7 4.3 .325 .206 .73 .53 .84 97.0 12.90 <t; +' Pl ~0 p:::J!2i L m ~ ~- (!) i :>: m (!) m ct! ôm 0 E-1 0 Q) m +' H P-1~ r-1 ~~ (!) <Dro ~·ri ~~ r-1 r-1 ::; Q) ..;tC ~s (1) ~0 ro os 3~ ct! +l Pim 0 ro C\l IJ:I "':R " ~~ r-1 :>:, NID ct!(!) ~(!) Or-1 (!.)r-I HO ,00 ~~ 1 ~ 1~-.::t C\l ..;t roo ·~ RW + ~..;t C\JO Pl s 0 0 (!.) R "':R r-1 1 0 (!.) rn .!si 33.8 5.10 8.20 - lOO - Table XIII tBe Decomposition of P.henyl n-Propyl Sulrihide vari§tion of k With Contact Time E:x:pt. No. T oA Contact Time k sec. sec.-1 49 847 0.252 0.237 34 848 0.965 0.262 47 859 0.262 0.440 32 859 0.925 0.423 7 883 0.273 1.14 31 883 0.935 1.19 18 894 0.276 1.84 29 894 0.900 1.50 58 902 0.226 2.18 39 902 0.894 2.07 56 927 0.082 5.10 61 927 0.295 5.14 - 101 Table XIV The Decomposition of Phenyl n-Propyl Sultihide variation of k with the Partial Pressure of Sultihide Sulphide Pressure k OA mm. Hg. sec.-1 36 839 0.105 0.175 37 839 0.295 0.205 33 846 0.039 0.226 34 848 0.095 0.262 20 868 0.118 0.669 21 870 0.315 0.718 30 895 0.033 1.49 29 894 0.096 1.50 6 913 0.027 3.75 1 913 0.058 3.52 14 927 0.052 5.50 15 927 0.285 5.87 Expt. No. T - 102 Table XV The Decomposition of Phenyl n-Propyl Su1phide variation of k with To1uene Pressure Expt. No. T oA To1uene Pressure k mm. sec.-1 Hg, 42 854 20.37 0.326 44 855 5.24 0.303 23 871 20.78 0.802 24 871 11.76 0.809 7 883 12.55 1.14 60 883 5.70 1.13 59 902 10.65 2.18 58 902 5.76 2.17 62 927 11.16 5.75 61 927 5.84 5.14 - 103 Table XVI The Decomposition of Phenyl n-Propyl Sultihide Effect of the Packed Reaction Vassel on k Expt. No. T k oA sec.-l 47 859 0.440 66P 859 0.400 7 883 1.14 65P 883 1.04 58 902 2.18 63P 902 2.29 14 927 5.50 64P 927 5.67 - 104 - C1 Phenyl Benzyl Sultihide Eroducts The main products of the decomposition, as shawn in Table XVII, were mercaptan, disulphide and dibenzyl. Mass spectroscopie analyses of the products collected in the trap maintained at -78°C showed that the mercaptan was exclusively phenyl mercaptan. Bath chemical and mass spectroscopie analyses indicated that dibenzyl, diphenyl disulphide and phenyl benzyl sulphide were the main products collected in the trap maintained at -5°C. At high reaction temperatures trace amounts of thiobenzophenone were identified by ultraviolet analysis (less than one per cent of the mercaptan and disulphide formed). Diphenyl disulphide, phenyl mercaptan and phenyl benzyl sulphide accounted for 99 per cent of .the sulphide pyrolyzed. The ratio of diphenyl disulphide to mercaptan varied from 0.8 to 0.08 over the temperature range from 759° to 880°K, decreasing with increasing temperature. The ratio of dibenzyl to mercaptan and disulphide varied from 0.5 to 1.0. - 105 - M§chanism of Decomposition The experimental results indicated that the primary step was the rupture of the C-S bond (1) with the formation of the phenylsulphide and benzyl radicals. The phenylsulphide radical not only reacted with toluene to form mercaptan (2) but also dimerized to form diphenyl disulphide (3) The benzyl radicals combined to give dibenzyl (4) At high reaction temperatures, small quantities of thiobenzophenone were produced, along with small amounts of non-condensible gases, presumably hydrogen. (5) To determine the extent of the recombination reaction (6) (6) - 106 two different approaches were employed. Initially, the recombination reaction was assumed to be negligible and first order rate constants were calculated from the amounts of mercaptan and disulphide formed. A plot of log k versus 1/T is shown in Figure 10, the straight line corresponding to an activation energy of 37.5 kcal./mole and a pre-exponential factor of 3 x 1010 sec.-1 The fact that this pre-exponential factor was much lower than that for the other C-S bond ruptures indicated that reaction (6) was indeed not negligible. Finally, to determine the extent of reaction (6) a series of pyrolyses were studied using toluene-oC-d as the carrier gas. Thus, deuterated 3 benzyl radicals were introduced into the system. An analysis of the pyrolyzed phenyl benzyl sulPhide, as shown in Table XVIII, revealed considerable amounts of the d2 component. Analysis of the dibenzyl produced gave a measure of the ratio of benzyl radicals to deuterated benzyl radicals in the system. This suggested that the recombination reaction was predominant, and that kinetic results based on mercaptan and disulphide were misleading. Bond Energies Although the kinetic study does not lead to a value for the bond energy, this may be calculated from thermo- - 107 chemical data. By use of Franklin's group method (139) a value can be derived for AHf(C 6H5ScH2C6H ). 5 AHf(C 6H 5 S-C~C 6 H 5 ) = lOAHf(~CH) + 2AHf()C-) +.ôHf(-S-) +AHf(CH2 ) = 10(3.30) + 2(5.57) + 11.6 - 4.9 = 50.9 kcal./mole Combination of this value with an average value of L:!.Hf(C6H5s) = 52.1 kcal./mole (see general discussion) and with the currently accepted value of 6 5 2 = 40 ~Hf(C H cH ) kcal./mole (5) yields a value of 41.1 kcal./mole for D(C 6H5S-CH2C6H5 ). - 108 - Figure 10 Plot of log k' vs. 1/T 1.0 0.5 .... ~ (.!) oo ....J ~5 1.15 .e ' 1.20 1/T X 103 1.25 1.30 - 109 - Table XVII Products of the decomposition of Phenyl benzyl sulphide e e (!) ra ro (!) +l p. 0 ex: () (!) m F-i P-t~ '0 § r •ri ..t;l p. .,.; :>;, o..ro «!Q) 1îro r-I ID Nl'f.l F-i .roo ,.; s ,00 ·ri +l Or-1 os 8S r-lr-1 :3 E-irn ~~ r-1 r-1 0 :3.-1 ~(!) ID r-I s ~ro rn + ~ p. s 0 () (L) A r-1 1 () (!) m ... ~~ 32 759 .17 6.85 262 .026 .016 - - 7.4 .45 21 766 .28 10.35 180 .055 .035 .031 • 35 18.7 .61 31 775 .15 6.95 270 .029 .024 - - 16 779 .29 10.20 156 .072 .046 .090 .77 24.5 .97 15 781 .30 8.95 116 .076 .048 - - 24.7 .95 30 798 .16 7.25 230 .047 .047 - - 18.9 1.33 20 807 .32 10.25 127 .258 .079 .325 .96 44.3 1.95 39 823 .21 5.80 133 .074 .045 - 37.2 2.20 38 824 .15 5.30 89 .165 .068 45.5 3.90 34 824 .13 4.40 90 .070 .056 - - 37.2 3.51 35 825 .14 5.00 322 .050 .019 - - 34.2 2.89 37 825 .16 4.80 159 .110 .107 - - 34.6 2.71 33 828 .14 6.60 263 .142 .063 .53 34.2 2.87 8 +l AS AS rn ~ .108 9.45 ~ .66 • e -!-) Pt ~0 Ml2i ct: 0 E-f 0 Q) rn -!-) rn rn Q) H P-i~ Q) § os r ri E-fS •ri ,.g Pt ri ri :3 ro ra -a rn ri ~~ mo s RS Q)ri ·ri ,.00 •ri 1 -!-) Pt li! ctiQ) Ori HO ·ri ria> :3ri ~ Nlil ~Q) s RS ro ~ro ;oi ·ll:l ro Pt s 0 0 Q) R ~ ri 1 0 Q) l1.l - ,!.:1 23 831 .27 9.80 127 .470 .075 .530 .97 61.0 3.50 25 833 .11 7.10 237 .158 .054 .128 .60 37.8 4.13 24 835 .13 5.50 120 .220 .145 .398 1.06 40.9 4.00 46 839 .45 5.60 66 .275 .050 - - 85.4 4.25 26 869 .10 7.40 322 .490 .046 .395 .74 67.9 10.8 28 875 .13 6.65 183 .565 .061 .474 . 76 80.0 12.2 29 880 .13 6.70 340 .332 .025 .280 . 79 80.6 12.5 - llO - Table XVIII Products of the decomposition of phenyl benzyl sulphide in toluene-cC -d3 .ç::.. j-I .ç::.. .ç::.. .ç::.. 0 .ç::.. \.N ()) ()) ()) -.J 1\) 1\) j-I .ç::.. .ç::.. 1..0 •j-I \.N • •1\) 0'\ 0 \.N ()) -.J ()) • IJ1 1\) jExpt No -.J IT OA .ç::.. ()) j-I 1..0 . . . . . IJ1 ()) 0'\ Q) IJ1 IJ1 IJ1 IJ1 j-I j-I j-I -.J 0 IJ1 j-I j-I 1\) 1\) .ç::.. j-I 1\) 0 0 0 0'\ \.N \.N 1..0 j-I -.J j-I \.N -.J \.N . . 1\) 0 0 Q) 1\) 1\) IJ1 \.N 0 0 • . . 0 0 \.N 0 \.N ~ 1\) \.N 1\) .p. 1\) 1\) 0 • . . . . 0'\ IJ1 1\) 0 0 0 0 \.N ()) -.J -..J 0 0 j-I lt sec Tol Press mm Hg 1\) . . . . . .ç::.. • 1..0 1\) Phenyl Benzyl Sulphide Pyrolyzed mmoles Mercaptan mmoles Disulphide mmoles . . . . . 0 0'\ 0 0 1..0 0 j-I j-I j-I \.N .p. IJ1 \.N .p. IJ1 1\) .p. 0 . . . . 0 0 1'\) 1..0 j-I j-I V1 1'\) 0 0 0 -.J IJ1 -..J \.N -..J ()) CD 1..0 1'\) CD CD 1\) ()) 1'\) j-I j-I 1\) 1'\) 1\) j-I 1..0 j-I V1 1..0 . . . . . 1..0 Phenyl Benzyl Sulphide Recovered After Pyrolys is mmoles ldo . •Q) • V1 j-I j-I \.N 1'\) 1\) 1'\) 0 -.J Q) j-I 1'\) • 0 •Q) -.J . . . . . d2 1o d 0 Dibenzyl l% d2 Dibenzyl 1% a4 Dibenzyl e - 111 - GENERAL DISCUSSION Experimental Errors The primary source of error in the determination of the rate constants was considered to be the measurement of the temperature of the reaction vessel during an experiment. of ± 1° The estimated fluctuation in temperature resulted in a considerable error in the rate constant. For example, as evaluated from the grapn in Figure 9, the rate constant for the decomposition of phenyl n-propyl sulphide at 900°A and 902°A was 2.09 sec. -1 and 2 •.24 sec. -1 , respectively. The error in the rate constant resulting from an uncertainty of 2° in the temperature is therefore about 7 per cent. The observed scatter in the rate constants may be explained for the most part by these fluctuations in temperature. For example, the differences between values of k for the two pairs of experimenta (42, 43) and (39, 58) done at 854°A and 902 0 A, respectively, are both 5 per cent. An error of 7 per cent in k would result in an error of less than 1 kcal./mole in the experimental activation energy as calculated from the slope of the plot of log k versus 1/T. The least favourable slope for the Arrhenius plot based on values of k with maximum scatter at both high and low - 112 temperature values would result in an error of less than 2 kcal~/mole in the experimental activation energy. In general, a factor of ± 2 kcal./mole was assigned to the activat~on energies determined for the thermal decompositions of phenyl ethyl sulphide and phenyl n-propyl suiphide. Dissociation Energies and He~ts of Formation of Radicale This study indicated the applicability of the toluene carrier technique for the determination of C-S bond dissociation energies in the phenyl alkyl sulphides. An essential requirement of this technique is that all radicale produced in the initial bond rupture be both sufficiently energetic and formed at a high enough temperature to react rapidly with toluene, thus preventing radical recombination reactions. In the etudies of the decomposition of both phenyl ethyl sulphide and phenyl n-propyl sulphide, the reaction of the phenylsulphide radical with toluene was found to be only moderately fast in the temperature range ·o 850°A to 950 A. To ensure complete removal of the phenyl- sulphide radicale from the system it was necessary to operate at toluene/sulphide ratios greater than 100:1. In the study of the decomposition of phenyl ethyl sulphide, the rate of C-S bond fission was measured by the rate of - 113 production of phenyl mercaptan rather than by the rate of productifn of c2 hydrocarbons, since ethyl radicals ' were apparently also removed from the system by combinationlwith benzyl radicals. This was not an entirely ideal procedure since some uncertainty existed as to whether all phenylsulphide radicale were converted to phenyl m'rcaptan, particularly under conditions favouring a high percentage of decomposition. In the decomposition of phenyl n-propyl sulphide, the n-pro.pyl radical decomposed completely to give ethylene plus a methyl radiJal, the rate of production of ethylene providing a more satisfactory measure of the rate of C-S bond fission. However, the consistency of the thermochemical values derived from both studies indicated the validity of either treatment. The fatlure of the toluene carrier technique in the study of the decomposition of phenyl benzyl sulphide was attributed to the comparative slowness of the reaction between the phenylsulphide radical and toluene at temperatures belo~ 850°A. The fact that the recombination rather than the abstraction process was predominant was shown by the formation of deuterated phenyl benzyl sulphide when benzyl radicals were produced in the system through the use of toluene-~-d 3 as a carrier gas. - 114 The frequency factors of 6 x 1014 and 8 x 1014 sec.- 1 determined for the rate constants of the C-S bond fissions in pnenyl ethyl sulphide and phenyl n-propyl sulphide, respectively, are similar and lie in the upper end of the 'normal' range for unimolecular reactions involving breakdown into two free radicals (145). Rate constants with frequency factors of 3 x 1014 and 3.3 x 1014 sec.-1 have previously been determined for C-S bond ruptures in phenyl methyl sulphide (115) and benzyl methyl sulphone (107). As proposed by Szwarc (1), the experimental activation energy can be identified with the bond dissociation energy within an uncertainty of RT. As previously discussed, the dissociation energy is not significantly different from the change in enthalpy at 25°C. Therefore, the experimental activation energies derived in this study were employed without correction in conjunction with the corresponding standard heats of formation at 25°0 to calculate the heat of formation of the phenylsulphide radical. An average value of 52.1 ±5 kcal./mole was proposed for the heat of formation of the phenylsulphide radical based on the values 52.4 and 53.0 kcal./mole obtained in this study and the value of 51.0 kcal./mole - 115 derived from the previous study of the decomposition of phenyl methyl sulphide (115). The Stability of the Ehenylsu1Phide Radical In both studies of the phenyl alkyl sulphide decompositions, a lower limit of 10.5 kcal./mole was determined for the resonance energy of the phenylsulphide radical from the expression The resonance stabilization is further supported by the strengthening of the c-s bond in the phenylsulphide radical with respect to that in the methylsulphide radical. The average value LlHf(c 6H s) = 52.1 kcal./mole together 5 with .6Hf(C 6H5 ) = 70 kcal./mole (5) and AHf(S) = 65.9 kcal./mole (146) leads to a value of D(C 6H5-s) mole as calculated from the expression = 84 kcal./ This value for the C-S bond dissociation energy in the phenylsulpnide radical is 16 kcal./mole higher than that proposed by Mackle (18) for the methylsulphide radical. - 116 - APPENDIX A Pyrolysis of Dirihenyl Disulrihide Introduction Presently accepted values for the S-S bond dissociation energies in disulpbides have been derived from the heats of formation of the alkylsulphide radicals and the gas phase heats of formation of the relevant disulphides. Sehon et al. (71) attempted to determine D(CH3S-SCH3 ) in a kinetic study of the thermal decomposition of dimethyl disulphide. However, the reaction was found to proceed by a molecular mechanism rather than by a free radical mechanism. A similar attempt was made in this investigation to determine D(C 6H S-SC 6H5 ) through a 5 kinetic study of the thermal decomposition of diphenyl d isulphide. Experimental The diphenyl disulphide was generously provided by Dr. Hawkins of Bell Telephone Laboratories, New Jersey, and was run without further purification. Pyrolysis in a toluene flow system at 765°K, 832°K, and 901°K indicated that the major products were mercaptan and dibenzyl. Small amounts of sulphide were identified • - 117 at the lowest reaction temperature. 0 The products collected in the trap at -5 C were dibenzyl, disulphide and sulphide, presumably benzyl phenyl sulPhide. The disulphide was determined by reduction to mercaptan with sodium borohydride followed by subsequent titration with O.lN silver nitrate using a platinum and mercurous sulphate electrode system (123). The sulphide was detected by titration with 0.05M potassium iodate in 90 per cent acetic acid using platinum and calomel electrodes (147). The method allowed an estimate of small amounts of sulphide to be made in large amounts of disulphide. The dibenzyl was not measured. The products collected in the trap at -78°C were mainly mercaptan. This was determined in the usual manner (125). Discussion The experimental results indicated that the primary step was the rupture of the S-S bond to give PhenylsulPhide radicals. (1) The phenylsulphide radicals reacted in part to give mercaptan, but the reaction was slow. (2) • - 118 Detection of a sulPhide not only indicated that the combination reaction (3) occurred to some extent, but also that some phenylsulphide radicals may have dimerized. (4) Thus, any kinetics based on the amount of mercaptan as an indication of the extent of bond breakage will be in error. However, if it is assumed that the bond breakage is a first order homogeneous process with a 'normal' pre-exponential factor of 101 3 sec.- 1 , an upper limit can be estimated for the bond energy by use of the Arrhenius equation. The average of the values so deriyed is D(c 6n5ssc 6H5 ) =· 48 kcal./mole (see Table XIX). The thermochemical values of ~Hf(c n s) = 52.1 = 58.4 D(c n s-sc 6n5 ) 6 5 6 5 kcal./mole and ~Hf(c 6 n5 ssc 6 ES) kcal./mole (148) allow the evaluation of since D(C 6H5ssc 6n5 ) = 2 liHf(C 6H5S) - LlHf(c 6n ssc 6H5 ) 5 • 2(52.1) - 58.4 • 45.6 kcal./mole - 119 - Although the experimental values are unreliable, they are at least of the correct arder of magnitude, indicating that the suggested mechanism is probable. - 120 - Table XIX Products of the decomposition of diphenyl disulphide e e Expt No T 0 t A sec To1uene Pressure To1uene Su1phide mm Hg Disu1phide mmo1es Pyro1yzed Recovered Mercaptan ~ Recovery (SS+SH) mmo1es k E sec-1 kca1/mo1e 1 901 .272 10.70 213 0.407 0.009 o. 729 91.7 8.25 49.5 2 832 .299 11.15 216 0.432 0.045 0.455 63.0 2.52 48.0 3 765 .375 11.65 160 0.505 0.360 0.130 84.0 0.37 47.0 - 121 - APPENDIX B Data and Calcu1ations for Experiment 20 (at 863°A) 1. Data A. P.hysical Measurements time of experiment (t) = 43.8 min. = 0.482 mmoles of sulphide = 3.675 moles of toluene = 131 moles of toluene moles of sulphide toluene pressure (p) = 1.175 reaction temperature (T) total number moles gases ~. Qhemical cm. = 863°A (n) = 0.486 MeAs~ements 1. Analysis of the contents of trap T1 : mmoles of sulphide = 1/2 x 50/25 x 0.102 x 2.85 = 0.290 (see Figure 6) weight of contents of trap Tl weight of sulphide weight of dibenzyl mmoles of dibenzyl 2. = 0.0910 = Q.0440 -- 0.0470 g. g. g. = 0.252 Analysis of the contents of trap T2: mmoles of mercaptan = 0.10 x 3.43 = 0.343 (see Figure 5) - 122 3. Analysis of the contents of trap T : 3 mmoles of condensible gases = 0.299 ratio of peak areas c2H4/C2H6 = 1.80 (measured from the gas chromatogram shown in Figure 7) 'fo C2H4 'fo C2H6 4. = 64.2 = 35.8 Analysis of the non-condensible gases: mmoles of non-condensible gases combustion analysis: P1 'fo 'fo 2. = 0.178 = 11.1 cm.; P2 = 3.7 CH4 = P2/P1 = 33.4 H2 = P1 - P2/Pl = 66.6 Calculations contact time (tc) = Y*(cc.) x p(cm.) x t(sec.) RxTxn = 201.5 x 1.175 x 2628 6234 x 863 x 0.486 = 0.238 sec. * V = volume of the reaction vessel rate constant (k) =~ tc ln _â_ a-x 1 ln 3.675 0.238 3.332 - 0.415 sec. -1 cm. - 123 - SUMMARY AND CONTRIBUTIONS TO KNOWLEDGE The thermal decompositions of phenyl ethyl sulPhide, phenyl n-propyl sulphide, and Phenyl benzyl sulPhide were studied using the toluene carrier technique. The products of the decomposition of phenyl ethyl sulphide were phenyl mercaptan, hydrogen, methane, ethane, ethylene and dibenzyl. The following mechanism was postulated to account for these products: c 6H5sc 2H5 ... ... C2HS C2H6 + c 6H5CH2 C2H4 + H C2H5 H + c 6H5cH3 H + C6H5CH3 t c 6H SH + c 6H5cH2 5 c 6H5S + c 6H5cH3 C2H5 + c 6H5cH3 c 6H5S 5 C6H c~ ... + H2 c 6H6 + CH3 C6IfsCH3 c 6H5cH2 + CH4 2C H C~ c ~cH CH c 6H CH3 t. 6 5 6 2 2 5 The rate constant for the first order, homogeneous decomposition of phenyl ethyl sulphide - 124 - as measured by the rate of production of phenyl mercaptan over the temperature range 843°A to 935°A was expressed by k = 6 x lo14 e- 59 , 500/RTsec.-l This activation energy was identified with D(c 6n s-c 2n ) and the heat of forma5 5 tion of the pbenylsulpbide radical was thus calculated to be 52.4 kcal./mole. The resonance energy of the phenyl- sulphide radical was estimated to be .). 10.5 kcal./mole. The products of the decomposition of phenyl n-propyl sulphide were phenyl mercaptan, ethylene, methane and dibenzyl. The mechanism was similar to that postulated for pbenyl ethyl sulphide with the exception that the n-propyl radical decomposed rapidly to form ethylene· anâ hyargg9I~. a metk~f rd tettl. .. The rate constant? as measured by the rate of production 0 0 of ethylene over the temperature range 832 A to 951 A was 14 -60,000/RT -1 expressed by k = 8 x 10 e sec. The activation energy was identified with D(c 6n s-n-c 3H?), and the heat 5 of formation of the phenylsulphide radical was calculated to be 53.0 kcal./mole. The resonance energy was again found to be .)- 10.5 kcal./mole. - 125 The products of the decomposition of phenyl benzyl sulphide were phenyl mercaptan, diprrenyl disulphide and dibenzyl. The following mechanism was postulated to account for these products. c H ScH2 C6~ 6 5 c 6H S + c 6H5CH 3 5 2C 6H5S 2C6H5CH2 - C H S + CH2C H 6 5 6 5 c H SH + 6 5 c H CH 6 5 2 c6H ssc 6H 5 5 c 6H5CH2CH2C6H5 However, appreciable decomposition occurred at low temperatures and under these conditions, the abstraction reaction with toluene was not sufficiently fast to prevent radical recombina ti on. Kinetic data based on the rate of production of phenyl mercaptan and diphenyl disulprride were misleading, and no dissociation energy could be d etermined. A similar mechanism was proposed for the decomposition of diphenyl disulphide based on preliminary experimente. Although mercaptan and dibenzyl were the chief products of the decomposition, no assurance could be given that the abstraction reaction proceeded rapidly enough in this temperature range to prevent radical recombination. - 126 BIBLIOGRAPHY il, 75 (1950). 1. Szwarc, M., Chem. Rev. 2. Cottrell, T.L., Strengths of Chemical Bonds, 2nd edition, Butterworths Scientific Publications, London, 1958. 52, 2826 (1922). 4. Skinner, H.A. and Pilcher, G., Quart. Rev. 11, 264 (1963). Ber.~' 3. Fajans, K., 643 (1920); 5. Skinner, H.A., R.I.C. Lectures, Monographs and Reports, No. 3 (1958). 6. Skinner, H.A., Rec. Trav. Chim. 12, 991 (1954). 7. Zahn, C.T., J. Chem. Phys. 8. Dewar, M.J.S. and Pettit, R.J., J. Chem. Soc. 1625 (1954). 9. Brown, R.D., J. Chem. Soc. 2615 (1953). ~' 671 (1934). ~' 10. Laidler, K.J., Can. J. Chem. 626 (1956). 11. Lovering, E.G. and Laidler, K.J., Can. J. Chem. 2a, 2367 (1960). 12. Tatevskii, V.M., Benderskii, V.A. and Yarovoi, s.s., nRules and Methods for Calculating the Physico-Chemical Properties of Paraffinic Hydrocarbons", translation ed. B.P. Mullins, Pergamon Press, Oxford, 1961. 13. Dewar, M.J.S. and Schmeising, H.N., Tetrahedron (1959); 14. 11, 96 (1960). Long, L.H., Quart. Rev. 2, 134 (1953). ~' 166 - 127 15. Reed, R.I. and Snedden, W., Trans. Faraday Soc. 2!, 301 {1958). 16. Thrush, B.A. and Zwolenik, J.J., Dise. Faraday Soc. 2!, 582 {1962). Soc.~' 17. Sehon, A.H., J. Am. Chem. 18. Mackle, H., Tetrahedron 19. Johns, J.W.C. and Ramsay, D.A., Can. J. Phys. ~' 4722 {1952). 1159 (1963). ~' 210 (1961). 20. JANAF Thermochemical Data, ed. D.R. Stull, Dow Chemical Co., Midland, Mich., 1961-1963. 21. Wieland, K., Helv. Chim. Acta. Z!, 1285 (1941). 22. Wieland, K., Z. Elektrochem. 23. Knox, B.E. and Palmer, H.B., Chem. Rev. 24. Brewer, L., Somayajulu, G.R. and Brackett, E., Chem. Rev. 25. ~' ~' 761 (1960). ~, 247 (1961). 111 (1963). Gaydon, A.G., Bond Dissociation Energies, Chapman and Hall, London, 1953. 26. Kerr, J.A., Sekhar, R.C. and Trotman-Dickenson, A.F., J. Chem. Soc. 3217 (1963). 27. Szwarc, M. and Taylor, J.W., Trans. Faraday Soc. !I, 1293 (1951). 28. Mortimer, C.T., Reaction Heats and Bond Strengths, Pergamon Press, London, 1962. li, 449 (1964). 29. Skinner, H.A., Ann. Rev. Phys. Chem. 30. Sehon, A.H. and Szwarc, M., Proc. Royal Soc. 202A, 263 (1950). - 128 31. Harrison, A.G. and Lessing, F.P., J. Am. Chem. Soc. ~~ 32. 519 (1960). Roberts, J.S. and Skinner, H.A., Trans. Faraday Soc. !i, 339 (1949). 33. Pauling, L., The Nature of the Chemical Bond, 3rd edition, Cornell University Press, 1960. 34. Wheland, G.W., Resonance in Organic Chemistry, Wiley, New York, 1955. ~' 35. Kandel, R.J., J. Chem. Phys. 1496 (1954). 36. Parks, G.S. and Vaughan, L.M., J. Am. Chem. Soc. ~' 2380 (1951). 37. Coulson, C.A., Theoretical Organic Chemistry, Butterworths, London, 1959. Soc.~' 38. Szwarc, M., Dise. Faraday 39. Jeffrey, G.A., Proc. Royal Soc. Al88, 222 (1947). 40. Ziegler, K., Seib, A., Knoevenagel, K., Herte, P. and Andreas, F., Annalen ~' 39 (1947). 150 {1942). Soc.~' 41. Pauling, L., J. Am. Chem. 42. Baughan, E.C., Evans, M.G. and Polanyi, M., Trans. Faraday 43. Soc.~' 988 (1932). 377 (1941). Trotman-Dickenson, A.F., Gas Kinetics, Butterworths Scientific Publications, London, 1955. A2, 44. Skinner, H.A., Trans. Faraday Soc. 45. Gowenlock, B.G., Polanyi, J.C. and Warhurst, E., Proc. Royal Soc.~' 269 {1953). 20 {1949). - 129 46. Carter, H.V., Chappe11, E.I. and Warhurst, E., J. Chem. Soc. 106 (1956). 47. Bi11ings, B.H.M. and Gowen1ock, B.G., Trans. Faraday Soc. 48. ~' Priee, S.J.W. and Trotman-Dickenson, A.F., Trans. Faraday 49. Soc.~' 939 (1957). Priee, S.J.W. and Trotman-Dickenson, A.F., Trans. Faraday 50. 690 (1963). Soc.~' 1208 (1957). Pilcher, G. and Skinner, H.A., J. Inorg. Nue. Chem. 2, 8 (1958). 51. Bichowsky, F.R. and Copeland, L.C., J. Am. Chem. Soc. 2Q, 1315 (1928). ~' 52. Cope1and, L.C., J. Am. Chem. Soc. 53. Franck, J., Trans. Faraday Soc. 54. KUhn, H., Z. Physik. 55. Leifson, 56. Birge, R.T. and Sponer, H., Phys. Rev. 28, 259 (1926). 57. Birge, R.T., Trans. Faraday 58. Beut1er, H., Z. phys. chem. B29, 315 (1935). 59. Buttenbender, G. and Herzberg, G., Ann. Physik. 21, s.w., ~' Zl, 2580 (1930). 536 (1925). 77 (1926). Astrophys. J. ~' 73 (1926). Soc.~' 707 (1929). 577 (1935). 60. Martin, E.V., Phys. Rev. !l, 167 (1932). 61. Terenin, A., Z. Physik. 21, 98 (1926). 62. Flory, P.J. and Johnston, H.L., J. Chem. Phys. 1!, 212 (1946). - 130 63. Colin, R., Goldfinger, P. and Jeunehomme, M., Trans. Faraday Soc.~' 306 (1964). 64. Stevenson, D.P., Dise. Faraday Soc. lQ, 35 (1951). 65. Berkowitz, J., J. Chem. Phys. 66. Hipple, J.A. and Stevenson, D.P., Phys. Rev. ~' 2533 (1962). ~' 121 (1943). 67. Stevenson, D.P., J. Chem. Phys. lQ, 291 (1942). 68. Franklin, J.L. and Lumpkin, H.E., J. Am. Chem. Soc . .ll., 1023 (1952). 69. Palmer, T.F. and Lessing, F.P., J. Am. Chem. Soc.~' 4 661 (1962). 10. Sehon, A.H. and Darwent, B. deB., J. Am. Chem. Soc. li_, 4806 (1954). 71. Braye, E.H., Sehon, A.H. and Darwent, B. deB., J. Am. Chem. Soc. 11, 5282 (1955). 72. Schissler, D.O. and Stevenson, D.P., J. Chem. Phys. 22, 151 (1954). 73. Farmer, J.B., Henderson, I.H.S., McDowell, C.A. and Lossing, F.P., J. Chem. Phys. 22, 1948 (1954). 74. Szwarc, M., J. Chem. Phys. 75. Rylander, P.N., Meyerson, Chem. 76. Soc.~' ~' s. 128 (1948). and Grubb, H.M., J. Am. 842 (1957). Perlman, M.L. and Rollefson, G.K., J. Chem. Phys. 362 (1941). ~' - 131 77. Herzberg, G., Molecular Spectra and Molecular Structure, I. Spectra of Diatomic Molecules, 2nd edition, Van Nostrand, New York, 1950. ~' 78. Langmuir, I., Phys. Rev. 329 (1913). 79. C1aasen, A. and Veenemans, C.F., Z. Physik. frQ, 342 (1933). 80. Knudsen, M., The Kinetic Theor,y of Gases, Methuen, London, 1934. ~~ 81. Wise, H., J. P.hys. Chem. 82. Chupka, W.A. and Inghram, M.G., J. Phys. Chem. (1955). 389 (1954). ~' 100 Porter, R.F., Chupka, W.A. and Inghram, M.G., J. Chem. Phys. ~' 216 (1955); ~' 1347 (1955); ~' 2159 (1955). 83. Honig, R.E., J. Chem. Phys. 22, 126 (1954); 22, 1610 (1954); 22, 1611 (1954). 84. Knight, H.T. and Rink, J.P., J. Chem. Phys. J2, 199 (1961). 85. Marquart, J.R. and Berkowitz, J., J. Chem. P.hys. ~~ 283 (1963). 86. Drowart, J., Exsteen, G. and Verhaegen, G., Trans. Faraday 87. Soc.~' 1920 (1964). Dwyer, R.J. and Oldenberg, O., J. Chem. Phys. 12, 351 (1944). 88. Bulewicz, E.M. and Sugden, T.M., Trans. Faraday Soc. ~' 720 (1959). - 132 89. Kistiakowsky, G.B., Knight, H.T. and Malin, M.E., J. Chem. Phys. 2Q, 876 (1952). go. Kistiakowsky, G.B. and Van Artsdalen, E.R., J. Chem. Phys. 91. ~. 469 (1944). Hormats, E.I. and Van Artsdalen, E.R., J. Chem. Phys. la, 778 (1951). 92. Fettis, G.C. and Trotman-Dickenson, A.F., J. Chem. Soc. 3037 (1961). 93. Corbett, P., Tarr, A.M. and Whittle, E., Trans. Faraday Soc.~' 94. 1609 (1963). Sehon, A.H. and Szwarc, M., Proc. Royal Soc. 209A, llO (1951). 95. Anderson, H.R., Jr., Scheraga, H.A. and Van Artsdalen, E.R., J. Chem. Phys. 96. ~' 1258 (1953). Sehon, A.H. and Szwarc, M., Ann. Rev. Phys. Chem. ~' 439 (1957). Soc.~' 97. Ogg, R.A., J. Am. Chem. 98. Sullivan, J.H., J. Phys. Chem. 99. Benson, 100. s.w. 526 (1934). ~' 722 (1961). and O'Neal, E., J. Chem. Phys. 21, 514 (1961). Flowers, M.C. and Benson, s.w., J. Chem. Phys. ~, Boyd, R.K., Downs, G.W., Gow, J.S. and Horrex, c., 882 (1963). 101. J. Phys. Chem. 102. ~' 719 (1963). Butler, E.T. and Po1anyi, M., Trans. Faraday 19 (1943). Soc.~' - 133 103. Steacie, E.W.R., Atomic and Free Radical Reactions, 2nd edition, Reinhold, New York, 1954. ~~ 104. Benson, S.W., J. Chem. Phys. 105. Blades, H., Blades, A.T. and Steacie, E.W.R., Can. J. Chem. ~~ 1945 (1963). 298 (1954). ~' 106. Takahasi, M., Bull. Chem. Soc. Japan 801 (1960). 107. Busfield, W.K. and Ivin, K.J., Trans. Faraday Soc. il, 1044 (1961). 108. Szwarc, M., J. Chem. Phys. 11, 505 (1949). 109. Szwarc, M., Ghosh, B.N. and Sehon, A.H., J. Chem. Phys. 18, 1142 (1950). llO. Szwarc, M., J. Chem. Phys. 11, 431 (1949). 111. Asheroff, S.J., Carson, A.S. and Pedley, J.B., Trans. Faraday Soc. 112. ~~ 2713 (1963). Ball, J.S., Encyclopaedia of Chemical Technology, Vol. 13, Interscience, New York, 1954. 113. Parker, A.J. and Kharasch, N., Chem. Rev. ~, 583 (1959). 114. Dainton, F.S. and Ivin, K.J., Quart. Rev. ~~ 61 (1958). 115. Back, M.H. and Sehon, A.H., Can. J. Chem. ~' 1076 (1960). Soc.~' 116. Cou1son, C.A., Dise. Faraday 9 (1947). 117. Mack1e, H. and Mayrick, R.G., Trans. Faraday Soc.~' 33 (1962). 118. Gowenlock, B.G., Kay, J. and Majer, J.R., Trans. Faraday Soc.~' 2463 (1963). - 134 119. Cook, G.L. and Foster, N.G., Froc. Am. Pet. Inst. Sect. III, !l, 199 (1961). 120. Earnshaw, D.G., Cook, G.L. and Dinneen, G.U., J. Phys. Chem. 121. ~' 296 (1964). Callear, A.B. and Cvetanovic, R.J., Can. J. Chem. 22, 1256 (1955). 122. Laitinen, H.A. and Kolthoff, I.M., J. Phys. Chem. !2, 1079 (1941). ~' 123. Stahl, C.R. and Siggia, S., Anal. Chem. 154 (1957). 124. Kolthoff, I.M., May, D.R., Morgan, P., Laitinen, H.A. and O'Brien, A.S., Ind. Eng. Chem., Anal. Ed. 18, 442 (1946). 125. Kolthoff, I.M. and Harris, W.E., Ind. Eng. Chem., Anal. Ed. 126. la, 161 (1946). Vogel, A.I., Quantitative Inorganic Analysis, 2nd edition, Longmans, London, 1951. 127. Leigh, C.H. and Szwarc, M., J. Chem. Phys. ZQ, 403 (1952). 128. Bywater, S. and Steacie, E.W.R., J. Chem. Phys. ~' 326 (1951). 129. Blades, A.T. and Steacie, E.W.R., Can. J. Chem. ~' 1142 (1954). ~' 130. Cher, M., J. Phys. Chem. 1316 (1964). 131. Kerr, J.A. and Trotman-Dickenson, A.F., Progress in Reaction Kinetics, Vol. 1, Pergamon Press, Oxford, 1961. • - 135 132. Benson, S.W., The Foundations of Chemical Kinetics, McGraw-Hill, New York, 1960. 133. Trotman-Dickenson, A.F. and Steacie, E.W.R., J. Chem. P.hys. ]a, 329 (1951). 134. Hubbard, W.N. and Waddington, G., Rec. Trav. Chim. ~' 135. 910 (1954). Bywater, S. and Steacie, E.W.R., J. Chem. Phys. 1&, 319 (1951). 136. •· Kerr, J.A. and Trotman-Dickenson, A.F., Trans. Faraday Soc. 52, 572 {1959). 137. Szwarc, M. and Taylor, J.W., J. Chem. Phys. 2310 ~' (1955). ~' 138. Mackle, H. and O'Hare, P.A.G., Tetrahedron 139. Franklin, J.L., Ind. Eng. Chem. !1, 1070 (1949). 140. Stevenson, D.P., Trans. Faraday 141. Calvert, J.G. and Sleppy, w.c., Soc.~' 611 (1964). 867 (1953). J. Am. Chem. Soc.~' 1544 (1959). 142. Kerr, J.A. and Calvert, J.G., J. Am. Chem. Soc.~' 3391 (1961). ~' 143. Brinton, R.K., J. Chem. Phys. 781 (1958). 144. Pope, A.E. and Skinner, H.A., Trans. Faraday Soc.~' 1404 (1964). li, 133 (1960). 145. Gowen1ock, B.G., Quart. Rev. 146. Mack1e, H. and O'Hare, P.A.G., Tetrahedron ~' 961 (1963). • - 136 Ga1'pern, G.D., Chemica1 Abstracts 148. Mack1e, H. and Mayrick, R.G., Trans. Faraday Soc • .5.a, 238 (1962) • • ~' 147. 10910 (1962).
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