JOURNAL OF CHEMICAL PHYSICS VOLUME 117, NUMBER 10 8 SEPTEMBER 2002 Rotational spectroscopy of 3 d transition-metal cyanides: Millimeter-wave studies of ZnCN „ X 2 ⌺ ¿ … M. A. Brewster and L. M. Ziurysa) Department of Astronomy, Department of Chemistry, and Steward Observatory, The University of Arizona, Tucson, Arizona 85721 共Received 5 April 2002; accepted 13 June 2002兲 The pure rotational spectrum of the ZnCN radical in its X 2 ⌺ ⫹ ground electronic state has been recorded using millimeter/sub-mm direct absorption techniques in the range 339–543 GHz. This work is the first spectroscopic observation of this molecule, which was created by the reaction of zinc vapor and cyanogen gas in a dc discharge. Twenty-one rotational transitions were recorded for the main zinc isotopomer, 64ZnCN, in its ground vibrational state, as well as 8 –16 transitions for the 66 Zn, 68Zn, and 13C isotopomers. Data was also obtained for ZnCN in several quanta of its bending mode and in the 共100兲 stretching vibration. These measurements indicate that the most stable form of zinc and the cyanide moiety is the linear cyanide structure, as has also been found for copper and nickel. In contrast, the linear isocyanide geometry is lowest in energy for gallium and aluminum. A spectroscopic analysis has been carried out of the 共000兲 and excited vibrational data, establishing (1) 兲 have rotational, spin-rotation, and l-type doubling parameters. Several structures 共r 0 , r s , and r m been determined for ZnCN as well, along with estimates of the heavy-atom stretch ( 1 ), and bending ( 2 ) frequencies. These calculations suggest that the metal–carbon bond in ZnCN is weaker than in CuCN or NiCN. The tendency of these metals to form the linear cyanide geometry, as opposed to the linear isocyanide or T-shaped structures, is additionally discussed. © 2002 American Institute of Physics. 关DOI: 10.1063/1.1498466兴 I. INTRODUCTION implications. Metal cyanide complexes are found in a variety of environments, including biological systems at enzyme sites,13 and in high-temperature superconductors.14 They also play a role in metal extraction for mining techniques,15 and in organic synthesis.16 Copper cyanide, for instance, is widely used in the creation of carbon–carbon bonds. Such varied use has inspired theoreticians to model the binding of the CN moiety on metal surfaces,17,18 as well as perform ab initio structural calculations of monomeric species.6 – 8 Transition metals are common in many of these environments. Yet, very little is known about the structures of monomeric transition metal cyanide/isocyanide complexes. Only recently have any of these species been investigated experimentally. Lie and Dagdigian, for example, have observed the FeNC molecule in the near UV by laser-induced fluorescence.11 These authors established that this radical has indeed the linear isocyanide structure in its most stable form. LIF studies have also been done very recently of NiCN by Merer and co-authors,19 who found that, in this case, the linear cyanide form was the ground state structure. In our group, we have measured the pure rotational spectrum of CuCN (X 1 ⌺ ⫹ ) using millimeter/submillimeter methods. A complete substitution structure was done on this molecule, unambiguously demonstrating that the ground electronic state has the linear cyanide geometry.20 Finally, we have also recorded the pure rotational spectrum of NiCN (X 2 ⌬ i ), verifying the work of Merer et al. and establishing lambdadoubling parameters.21 It is interesting to note that iron prefers the isocyanide geometry, but for nickel and copper, the cyanide species is the lower-energy configuration. At gal- One of the more interesting chemical systems are the metal–cyanide complexes. These species in their simplest, monomeric form can exhibit three distinct geometries: a linear cyanide compound, a linear isocyanide, and a T-shaped, quasistructureless molecule.1–5 As theorists have described, the dominance of a particular geometry depends on the balance between columbic attraction and exchange repulsion, and electronegativity of the metal involved.6 –9 In the alkali group, the metal is thought to completely give its valence electron to the cyanide moiety, generating an M⫹ CN⫺ structure in which the M⫹ ion orbits the CN⫺ group with no preference for a particular bonding site.1,2,6 Hence, a T-shaped structure is generated with a highly ionic bonding scheme. The alkaline earth metals tend to form linear isocyanides,3,9,10 where the metal atom is attached at the negatively polarized nitrogen end of the CN group. There is then a covalent contribution to the bonding. It is thought that if covalent bonding dominates, then the linear cyanide species is expected, analogous to HCN.6 – 8 Therefore, for certain metals, the cyanide form might be the lowest-energy structure. Until recently, experimental work has proved otherwise; aluminum,4,5 iron,11 gallium,12 and even indium,12 for example, have all been shown to favor the isocyanide geometry in their ground state. NaCN and KCN adopt the T-shaped structure.1,2 Establishing the geometries of metal cyanide species, particularly in their monomeric form, has many chemical a兲 Electronic mail: [email protected] 0021-9606/2002/117(10)/4853/8/$19.00 4853 © 2002 American Institute of Physics Downloaded 31 Aug 2002 to 128.196.209.95. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/jcpo/jcpcr.jsp 4854 J. Chem. Phys., Vol. 117, No. 10, 8 September 2002 M. A. Brewster and L. M. Ziurys lium, the linear isocyanide species is again favored.12 In order to further examine the trends in transition metal/CN bonding, we have measured the pure rotational spectrum of ZnCN. This study is the first spectroscopic observation of this molecule. A wide range of rotational transitions were recorded for the main isotopomer, 64ZnCN, as well as for 66ZnCN, 68ZnCN, and 64Zn 13CN. Transitions arising from several of the vibrationally excited states were observed in the zinc isotopomers as well. This free radical was also found to be linear and exists as a metal cyanide in its lowest-energy configuration, with a 2 ⌺ ⫹ ground electronic state. Spectroscopic constants, vibrational frequencies, and bond lengths have been established for ZnCN. Here we present these results and discuss them in the context of metal cyanide/isocyanide complexes. II. EXPERIMENT The measurements were made with one of the quasioptical millimeter/sub-mm spectrometer systems of the Ziurys group. This instrument consists of a Gunn oscillator/varacter multiplier source, a reaction chamber containing a Broidatype oven for metal vaporization, and an InSb hot electron bolometer detector. The system is under computer control. Phase-sensitive detection is achieved by FM modulation of the Gunn oscillator. For more details, see Ref. 22. ZnCN was produced in a dc glow discharge using a mixture of 25–30 mTorr argon, 3–5 mTorr cyanogen, and ⬍1 mTorr zinc vapor, produced from the Broida-type oven. A similar synthetic technique was previously used in our studies of AlNC,4 MgCN,23 and CuCN.20 The reactant and carrier gases were premixed and introduced from beneath the oven to produce the molecule. Mossy zinc was found to be an acceptable material to use for the purposes of this synthesis. The typical discharge voltage used was 400 V, producing 90 mA of current through the reaction mixture. The discharged gas typically was purple in color due to argon. Three zinc isotopomers of ZnCN were observed in their natural abundances ( 64Zn: 66Zn: 68Zn⫽48.9:27.8:18.6). The signal-to-noise of the spectra, however, was insufficient to record data for the 13C species in its natural abundance. Therefore, H13CN was substituted for the cyanogen as the precursor for Zn13CN. Typically 1–3 mTorr H13CN was used in an effort to minimize the amount of starting material consumed. H13CN was synthesized for this purpose by the slow addition of concentrated sulfuric acid to a concentrated aqueous solution of Na13CN 共Cambridge isotopes兲, under a continuous flow of helium, introduced to the reaction vessel from beneath the surface of the solution. The stream of gas was subsequently flowed through anhydrous calcium sulfate and then over P2 O5 to dry it. Finally, the H13CN was collected in a liquid nitrogen-cooled glass bulb fitted with a valve. Upon warming to room temperature the material was ready for use. Actual transition frequencies were measured from spectra that were an average of two scans. One scan was taken in increasing frequency and the other in decreasing frequency over the same range. Signals were found to be sufficiently strong such that only one average was necessary for all mea- FIG. 1. A stick figure illustrating the positions and approximate relative intensities of the spectral lines observed in the N⫽59→60 rotational transition of ZnCN (X 2 ⌺ ⫹ ). The spin-rotation splitting has been neglected for simplicity. Lines originating from the main zinc isotopomer, 64ZnCN, in both its ground vibrational state 共000兲, several quanta of the v 2 bending mode, and the v 1 ⫽1 stretching vibration, are present in the spectrum. Also visible in the data are the 共000兲 and 共010兲 states of the less abundant zinc isotopomers, 68ZnCN and 66ZnCN, and the ground vibrational state of the 13 C isotopomer. The v 2 vibrational satellite lines are all split by l-type effects of varying magnitude, as illustrated in the figure. surements. Linewidths were typically 700–1200 kHz over the range 330–544 GHz. III. RESULTS ZnCN had not been observed previously by any other experimental method; nor had any ab initio calculations been performed for this molecule. It was consequently unclear at the start of the study whether the species was bent or linear, or whether the cyanide or isocyanide form would be the dominant structure. To attempt to measure its spectrum, it was assumed that the molecule was linear and had a 2 ⌺ ⫹ ground state. A rotational constant of ⬃4 GHz was then estimated by scaling from that of CaNC by mass. A spinrotation constant of ⬃100 MHz was also predicted based on that of ZnCH3 24 and using the ratio of spin-rotation constants of MgNC and MgCH3 as a scaling factor.3,25 A range of ⬃2B 共⬃8 –9 GHz兲 was then scanned in frequency space in 100 MHz sections. Doublets were found in these data with approximately the estimated fine structure splitting. Harmonic relationships were then predicted and other matching transitions identified, in the process establishing the correct rotational quantum numbers. Effective rotational parameters were then accurately determined for the three zinc isotopomers in their ground vibrational state and several excited vibrational states, such that additional transitions could be readily predicted and measured. It was obvious at this point that the molecule was linear; measurements of transitions of the 13C isotopomer established that the radical was ZnCN, as opposed to ZnNC. A stick figure of the rotational lines observed for ZnCN within a given transition (N⫽59→60) with approximate Downloaded 31 Aug 2002 to 128.196.209.95. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/jcpo/jcpcr.jsp J. Chem. Phys., Vol. 117, No. 10, 8 September 2002 Millimeter-wave studies of ZnCN 4855 TABLE I. Observed transition frequencies of ZnCN (X 2 ⌺ ⫹ :(000)).a 64 66 ZnCN 68 ZnCN Zn13CN ZnCN N⬙ N⬘ J⬙ J⬘ obs o–c obs o–c obs o–c obs o–c 43 44 44 45 45 46 46 47 47 48 48 49 49 50 50 51 51 52 56 57 57 58 58 59 59 60 60 61 61 62 62 63 63 64 64 65 65 66 66 67 67 68 68 69 69 70 70 71 42.5 43.5 43.5 44.5 44.5 45.5 45.5 46.5 46.5 47.5 47.5 48.5 48.5 49.5 49.5 50.5 50.5 51.5 55.5 56.5 56.5 57.5 57.5 58.5 58.5 59.5 59.5 60.5 60.5 61.5 61.5 62.5 62.5 63.5 63.5 64.5 64.5 65.5 65.5 66.5 66.5 67.5 67.5 68.5 68.5 69.5 69.5 70.5 43.5 44.5 44.5 45.5 45.5 46.5 46.5 47.5 47.5 48.5 48.5 49.5 49.5 50.5 50.5 51.5 51.5 52.5 56.5 57.5 57.5 58.5 58.5 59.5 59.5 60.5 60.5 61.5 61.5 62.5 62.5 63.5 63.5 64.5 64.5 65.5 65.5 66.5 66.5 67.5 67.5 68.5 68.5 69.5 69.5 70.5 70.5 71.5 339 574.263 339 676.998 347 269.472 347 372.165 354 963.088 355 065.693 362 655.044 362 757.618 ¯ ¯ 378 034.006 378 136.433 385 720.899 385 823.277 393 406.033 393 508.324 401 089.364 401 191.591 439 477.758 439 579.613 447 149.540 447 251.322 454 819.279 454 920.965 462 486.908 462 588.545 470 152.450 470 254.001 477 815.820 477 917.286 485 477.020 485 578.382 493 135.982 493 237.264 500 792.687 500 893.882 508 447.086 508 548.198 516 099.167 516 200.176 523 748.885 523 849.809 531 396.212 531 497.058 ¯ ¯ ¯ ¯ 0.032 0.022 0.037 0.045 0.039 0.020 0.005 0.019 ¯ ¯ 0.005 0.001 ⫺0.005 0.010 ⫺0.007 ⫺0.011 ⫺0.010 ⫺0.009 ⫺0.025 ⫺0.028 ⫺0.025 ⫺0.024 ⫺0.019 ⫺0.035 ⫺0.039 ⫺0.023 ⫺0.026 ⫺0.014 ⫺0.029 ⫺0.019 ⫺0.013 ⫺0.022 ⫺0.008 ⫺0.012 0.001 ⫺0.003 0.000 0.001 0.012 0.001 0.030 0.024 0.058 0.067 ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ 397 818.102 397 919.492 ¯ ¯ 443 504.282 443 605.196 451 111.756 451 212.632 458 717.232 458 818.019 466 320.574 466 421.312 473 921.825 474 022.476 481 520.905 481 621.481 489 117.800 489 218.296 496 712.510 496 812.883 504 304.903 504 405.216 511 895.043 511 995.256 519 482.828 519 582.968 527 068.260 527 168.283 534 651.296 534 751.233 542 231.866 542 331.735 ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ 0.033 0.040 ¯ ¯ 0.023 ⫺0.015 ⫺0.011 ⫺0.011 0.009 ⫺0.002 ⫺0.018 0.000 ⫺0.015 ⫺0.003 ⫺0.026 ⫺0.008 ⫺0.031 ⫺0.010 0.004 ⫺0.013 ⫺0.016 ⫺0.009 0.006 0.000 0.003 0.012 0.012 ⫺0.006 0.025 0.011 0.007 0.017 ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ 364 474.364 364 575.263 ¯ ¯ 379 606.958 379 707.717 387 170.704 387 271.388 394 732.695 394 833.326 ¯ ¯ 440 066.087 440 166.289 447 614.841 447 714.993 455 161.619 455 261.723 462 706.382 462 806.349 470 249.020 470 348.932 477 789.546 477 889.333 485 327.902 485 427.624 492 864.047 492 963.703 500 398.018 500 497.532 507 929.701 508 029.159 515 459.089 515 558.438 522 986.131 523 085.416 530 510.882 530 609.951 538 033.131 538 132.244 ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ 0.045 0.035 ¯ ¯ 0.033 0.013 0.028 0.001 0.016 0.005 ¯ ¯ 0.010 0.010 ⫺0.046 ⫺0.018 ⫺0.056 0.004 ⫺0.025 ⫺0.021 ⫺0.029 0.003 ⫺0.019 ⫺0.030 ⫺0.021 ⫺0.012 ⫺0.041 ⫺0.011 ⫺0.007 ⫺0.031 0.001 0.009 0.010 ⫺0.001 0.004 0.020 0.071 ⫺0.036 0.034 0.066 ¯ ¯ 343 455.845 343 557.411 351 065.036 351 166.550 358 672.637 358 774.089 366 278.612 366 380.013 373 882.913 373 984.243 ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ 525 564.381 525 664.138 533 125.549 533 225.199 540 684.247 540 783.827 ¯ ¯ 0.020 0.010 0.000 ⫺0.002 ⫺0.009 ⫺0.010 ⫺0.007 0.004 ⫺0.008 ⫺0.003 ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ ¯ 0.006 0.007 0.012 ⫺0.002 ⫺0.014 ⫺0.004 a In MHz. relative intensities is shown in Fig. 1. The splittings due to fine structure are neglected. For the main isotopomer ( 64ZnCN), the ground vibrational state and lines originating from the v 2 ⫽1, 2, and 3 quanta of the bending mode were observed, as well as the first quantum of the heavy-atom stretch 共100兲. The 共010兲 and 共020兲 levels show the effects of l-type doubling and l-type resonance. Also present are the 共000兲 and 共010兲 vibrational states of the 66ZnCN and 68ZnCN isotopomers, which are weaker in intensity. The weakest signal recorded arises from Zn13CN in its ground vibrational state. The vibrational satellite pattern is typical for a linear, reasonably rigid triatomic molecule. The (011 0), (022 0), and (033 0) states are regularly spaced in frequency with respect to the 共000兲 state, with ␣ 2 ⬍0. Also, the (020 0) line has not significantly shifted away from the (022 0) features, as occurs when a molecule is quasilinear.26 Table I presents the transition frequencies of the four isotopomers observed 共64ZnCN, 66ZnCN, 68ZnCN, and 64 Zn13CN兲 in their ground vibrational state. Between 8 and 21 transitions were recorded for each species. In every transition measured, the spin-rotation splitting was resolved, which varies from about 98 to 103 MHz. Between 10–12 Downloaded 31 Aug 2002 to 128.196.209.95. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/jcpo/jcpcr.jsp 4856 J. Chem. Phys., Vol. 117, No. 10, 8 September 2002 M. A. Brewster and L. M. Ziurys FIG. 2. Spectrum of the N⫽48→49 rotational transition of 64ZnCN(X 2 ⌺ ⫹ ) near 378 GHz, observed in its ground vibrational state. The transition consists of doublets, labeled by quantum number J, which arise from spin– rotation interactions and indicate that this molecule has a 2 ⌺ ⫹ ground state. This spectrum is a composite of two single 100 MHz scans, each acquired in approximately one minute. FIG. 3. Observed spectrum of the N⫽51→52 rotational transition of the 68 ZnCN isotopomer near 395 GHz in its ground vibrational and electronic states, measured in natural abundance ( 64Zn: 68Zn⫽48.9:18.6). The line marked by an asterisk is an unidentified feature. The spin–rotation doublets, labeled by the J quantum number, are clearly resolved in these data. This spectrum is a composite of two single 100 MHz scans, each recorded in about one minute. TABLE II. Molecular constants for ZnCN (X 2 ⌺ ⫹ :( v 1 v 2 v 3 )). a ( v 1v 2v 3) Parameter 共000兲 B D ␥ ␥D B D H(109 ) ␥ ␥D q qD p B D H(109 ) ␥ ␥D B D H(109 ) ␥ ␥D q eff q D eff(108 ) B D H(109 ) ␥ ␥D q eff(109 ) B D H(109 ) ␥ ␥D rms of fit 共010兲 (020 0) (022 0) (033 0) 共100兲 64 ZnCN 3865.08340 共86兲 0.001 472 52 共12兲 104.05 共18兲 ⫺0.000 225 共17兲 3892.5528 共42兲 0.001 588 9 共12兲 0.63 共12兲 102.87 共17兲 ⫺0.000 205 共15兲 ⫺6.003 1 共16兲 0.000 032 21 共20兲 ⫺0.482 共93兲 3910.857 共19兲 0.001 9750 共48兲 ⫺0.75 共40兲 102.58 共47兲 ⫺0.000 215 共41兲 3920.466 4 共43兲 0.001 685 0 共12兲 0.22 共11兲 100.98 共23兲 ⫺0.000 147 共20兲 ⫺0.000 052 02 共38兲 0.2141 共60兲 3948.8362 共58兲 0.001 817 0 共16兲 1.09 共14兲 98.52 共32兲 ⫺0.000 063 共27兲 ⫺0.1731 共78兲 3855.403 0 共76兲 0.001 265 4 共20兲 4.19 共17兲 103.43 共41兲 ⫺0.000 229 共35兲 0.044 66 68 ZnCN ZnCN Zn13CN 3833.5004 共14兲 0.001 449 58 共18兲 103.15 共36兲 ⫺0.000 217 共29兲 3860.7352 共47兲 0.001 564 4 共13兲 0.64 共11兲 102.06 共24兲 ⫺0.000 205 共20兲 ⫺5.905 9 共22兲 0.000 031 29 共26兲 ⫺0.494 共93兲 3803.7148 共11兲 0.001 428 34 共13兲 102.45 共24兲 ⫺0.000 223 共20兲 3830.7233 共76兲 0.001 540 9 共19兲 0.61 共16兲 101.39 共28兲 ⫺0.000 209 共22兲 ⫺5.814 0 共24兲 0.000 030 30 共28兲 ⫺0.483 共95兲 3822.617 63 共99兲 0.001 451 24 共12兲 102.92 共20兲 ⫺0.000 222 共19兲 0.034 0.030 0.009 In MHz; errors quoted are 3 and apply to the last quoted decimal places. a Downloaded 31 Aug 2002 to 128.196.209.95. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/jcpo/jcpcr.jsp J. Chem. Phys., Vol. 117, No. 10, 8 September 2002 Millimeter-wave studies of ZnCN TABLE III. Vibrational dependence of B v . a ZnCN (X 2 ⌺ ⫹ ) Parameter a TABLE V. Bond lengths for transition metal cyanides. CaOH (X 2 ⌺ ⫹ ) b 3835.6644共12兲 ⫺31.5974 共6兲 ⫺2.1778 共4兲 2.4029共10兲 B̃ e ␣2 ␥ 22 ␥u 4857 MgOH (X 2 ⌺ ⫹ ) b ¯ 31.518共3兲 2.849共3兲 ⫺3.361共1兲 14 911.76共10兲 110.47 共5兲 21.18 共3兲 18.27 共3兲 In MHz. Reference 26. b Species a CuCN ZnCN GaCNb rotational transitions were also recorded for 64ZnCN in its (011c 0), (011d 0), (020 0), (022c 0), (022d 0), (033c 0), (033d 0), and 共100兲 vibrational states, and for the 66Zn and 68 Zn isotopomers in their (011c 0) and (011d 0) levels. These data are available via EPAPS.27 The l-type doubling in the 共010兲 state typically ranges from 550 to 800 MHz, while in the 共020兲 state it is much smaller 共⬃20–50 MHz兲, as expected. In the 共030兲 level, the l-type splitting is collapsed at the lower-N transitions observed, but is resolved at higher N, where the separation between the c and d components is, at most, 1–2 MHz. Representative spectra of the ZnCN radical are shown in Figs. 2 and 3. Figure 2 presents the N⫽48→49 rotational transition in the 共000兲 vibrational mode of the main zinc isotopomer, 64ZnCN, near 378 GHz. The spin–rotation doublets are clearly present in the spectrum, and are labeled by quantum number J. Figure 3 shows the N⫽51→52 rotational transition of 68ZnCN in its ground vibrational mode near 394 GHz, observed in the natural zinc abundance ratio of 64Zn: 68Zn⫽48.9:18.6. An unidentified line in the data is marked by an asterisk. Again, the fine structure doublets are clearly visible in the spectrum. Curiously, the signal-to-noise ratio in these data does not vary significantly from that of 64 ZnCN 共Fig. 2兲, although the zinc abundance differs by a factor of 2.6. Such variations in signal are typical in this case and reflect the fluctuations in molecule production of elusive free radicals. IV. ANALYSIS The data for all isotopomers of ZnCN observed in their ground vibrational state and the 共100兲 stretching mode were analyzed using a simple Hamiltonian consisting of molecular frame rotation and spin-rotation coupling, including their centrifugal distortion corrections: Ĥ eff⫽Ĥ rot⫹Ĥ sr . 共1兲 a Structure r0 rs r m(1) r0 rs r m(1) r0 rs r m(1) r M–C 共Å) 1.8323 1.8328 1.8358 1.9545 1.9525 1.9496 2.0616共4兲 2.059 2.058 r C–N 共Å) 1.1576 1.1567 1.1573 1.1464 1.1434 1.1417 1.1580共6兲 1.160 1.160 Reference 20. Reference 12. b For the excited bending states, however, the effects of l-type doubling and l-type resonance had to be considered. As discussed in Apponi, Anderson, and Ziurys,26 these interactions are quite simple for the 共010兲 state because they only involve l-type doubling and an energy term in q, the l-type doubling constant. For the higher quanta of the bending mode, on the other hand, the l-type interactions include off-diagonal terms varying by l⫾4 as well as l⫾2, and hence require matrix representation. In the construction of these matrices, a knowledge of the energy separation between the l subcomponents of a given v 2 level is additionally needed. This information is not presently available for ZnCN, and therefore the l-type interactions in the v 2 ⫽2 and 3 states could only be modeled using an effective term with a corresponding constant, q eff . 共For exact energy expressions, see Ref. 26.兲 Finally, a p term was found necessary for the 共010兲 state analysis to account for differences in spin-rotation splittings between the l-type doublets, c and d. This correction has the same functional form as the lambda-doubling constant p in ⌸ states.26 The molecular constants determined for the four isotopomers of zinc cyanide, 64ZnCN, 66ZnCN, 68ZnCN, and 64 Zn13CN, are listed in Table II. This table also includes the parameters established for the 共010兲, (020 0), (022 0), (033 0), and 共100兲 vibrational states. As is evident in the table, centrifugal distortion corrections to ␥ and q 共␥ D , q D , and q Deff兲 were found necessary in most of the analyses. 共One most global fit was done for all data for each isotopomer.兲 All resulting constants were well determined, and the individual rms of each data was better than 45 kHz 共see Table II兲. V. DISCUSSION A. Structural properties of ZnCN „ X 2 ⌺ ¿ … TABLE IV. Derived vibrational frequencies of transition metal cyanides.a 1 (expt.) NiCN CuCN ZnCN GaCN In cm⫺1 Reference 21. c Reference 20. a b b 496 478c 418 348e 1 共ab initio兲 2 (expt.) 2 共ab initio兲 ¯ 453d ¯ 339f ¯ 270c 212 ¯ ¯ 225d ¯ 112f d Reference 32. Reference 12. f Reference 31. e This study has shown that the most stable form of zinc and the cyanide moiety is the linear cyanide structure, ZnCN. Hence, zinc behaves similarly to the other later 3d transition metals that have been investigated, copper and nickel.19–21 For gallium, the next element after zinc, the favored geometry is linear GaNC. The isocyanide structure is also found for iron. This structural alternation will be discussed later. Not only does zinc bond to the carbon as opposed to the nitrogen in CN, but it forms a relatively rigid, linear structure as well. Evidence for rigidity is found in the vibrational pro- Downloaded 31 Aug 2002 to 128.196.209.95. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/jcpo/jcpcr.jsp 4858 J. Chem. Phys., Vol. 117, No. 10, 8 September 2002 M. A. Brewster and L. M. Ziurys gression, as already discussed and shown in Fig. 1. Quantitatively, this vibrational sequence can be modeled using an expression for the dependence of B v on v 2 , the bending mode quantum number:26 B v ⫽B̃ e ⫺ ␣ 2 共 v 2 ⫹1 兲 ⫹ ␥ 22共 v 2 ⫹1 兲 2 ⫹ ␥ ll , 共2兲 where B̃ e ⫽B e ⫺ 12 ( ␣ 1 ⫹ ␣ 3 ). Using the 共000兲, (011 0), (022 0), (020 2), and (033 0) data, the four constants in Eq. 共2兲 have been determined for ZnCN and are presented in Table III. Also listed in this table are a similar set of constants derived for rigid, linear CaOH, and quasilinear MgOH.26 As this comparison demonstrates, the ␥ 22 and ␥ ll constants that reflect the deviations from linearity, are very similar in magnitude for ZnCN and CaOH, although the signs change. In contrast, those of MgOH are about a factor of 10 larger. ZnCN consequently does not appear to show much evidence for quasilinear behavior. CuCN also appears to be fairly rigid, as suggested by its regular vibrational progression.20 GaNC, in contrast, exhibits large-amplitude bending motions, which indicate a flat bending potential.12 Evidence for such a potential is found in the unusually short N–C bond distances for GaNC 关r 0 ⫽1.1494(46) Å and r s ⫽1.1419(80) Å兴. The value in HNC (2) is closer to 1.16 –1.17 Å. The calculation of an r m structure for GaNC, which takes into account zero-point vibrations,28 appears to correct this anomalously short bond length, yielding r N–C⫽1.1629 共1兲 Å—more in the range of usual values.12 InCN also appears to exhibit a very short N–C bond length and an even flatter bending potential.12 Although the geometry of ZnCN is linear, it does not appear to be as strongly bonded as its copper or nickel analogs. This characteristic is apparent in calculated vibrational frequencies for the metal–carbon stretch ( 1 ) and the bend ( 2 ) in these molecules. The heavy atom stretching frequency can be estimated by treating the CN moiety as a unit and using the approximate relationship for diatomic molecules:29 1⬇ 冑 4B 30 D0 共3兲 . The bending mode vibration can be derived from the l-type doubling constant q via the relationship:30 q⫽ ⫺2B 2e 2 冉 1⫹4 2 2i 22 兺i 2i ⫺ 22 冊 . 共4兲 The last term in this equation, the Coriolis term, is usually near 0.3, so the above expression simplifies to30 q⬇ 2.6B 2e 2 . 共5兲 In the case of CuCN and ZnCN, B e itself could not be derived, so B̃ e was used instead. The resulting vibrational frequencies calculated for ZnCN are listed in Table IV, along with those derived for CuCN,20 NiCN,21 and GaCN,12 if available. 共Ab initio values have also been computed for two of these molecules31,32 and are given in Table IV as well. They are in good agreement with those derived from experimental data and the above approximations.兲 As shown, the metal–carbon stretch for ZnCN was found to be 1 ⬇418 cm⫺1 as opposed to 478 and 496 cm⫺1 for CuCN and NiCN, respectively. Hence, the stretching frequency decreases considerably in going from CuCN to ZnCN, indicating a weakening of the metal–carbon bond. Such an effect might be expected, because CuCN is closed shell (X 1 ⌺ ⫹ ) while ZnCN is a radical (X 2 ⌺ ⫹ ). On the other hand, NiCN is a radical as well, with a 2 ⌬ i ground state, yet the metal–carbon stretching frequency is comparable to that of CuCN. The Ga–C stretch is lower in energy than that of ZnCN, with 1 ⬇348 cm⫺1 , suggesting an even weaker bond. Given that GaNC is the more stable geometry, this decrease is not unexpected. Experimentally derived bending mode frequencies are only available for CuCN and ZnCN. Again, the bending frequency decreases in going from copper ( 2 ⬇270 cm⫺1 ) to zinc ( 2 ⬇212 cm⫺1 )—another indication that ZnCN is not as strongly bound as CuCN. A theoretical calculation of 2 is available from the literature for GaCN,31 and this value 共112 cm⫺1兲 is almost half that of ZnCN. 共An ab initio estimate has also been obtained for CuCN: 2 ⬇225 cm⫺1 , fairly close to the experimental value of 270 cm⫺1.32兲 Because isotopic substitutions were carried out for the (1) structures zinc and carbon atoms on ZnCN, r 0 , r s , and r m can be calculated. These results are given in Table V, along with those derived for GaCN and CuCN. The r 0 and r s geometries are determined, respectively, by a least-squares fit to the moments of inertia (r 0 ) and to Kraitchman’s equations (1) structure was derived using the method (r s ), 33 while the r m employed by Watson.28 In the latter case, the experimentally determined moments of inertia were fit to the expression I 0 ⫽I m ⫹c 冑I m , 共6兲 where I m are the rigid, mass-dependent moments of inertia and c is a constant. The second term in the above equation is thought to, in part, correct for zero-point vibrations; hence, (1) structure is thought to be superior to both r 0 and r s an r m (2) geometries. 共The derivation of an r m structure would have been preferable because it is thought to be closest to the equilibrium geometry.28 This calculation was not possible because it requires the substitution of all atoms, which was not done for ZnCN.兲 As shown in Table V, the zinc–carbon bond length is r (1) ⫽1.9496 Å). ⬇1.95 Å, as indicated by all structures (r m The C–N bond distance varies over the range 1.1417 Å (1) ) to 1.1464 Å (r 0 ). The metal–carbon bond length in (r m ZnCN is intermediate in value between that of CuCN 共1.8358 Å兲 and GaCN 共2.058 Å兲, as might be expected. In contrast, the C–N bond distance in ZnCN appears to be anomalously short—both bond lengths in CuCN and GaCN are significantly longer 共1.157–1.160 Å兲, and are comparable to that in HCN 共1.1540 Å12兲. An unusually short C–N bond of 1.143–1.146 Å has (1) structures. In also been found in InCN,12 based on r s and r m (2) structhis case, all atoms were substituted such that an r m ture could also be derived, which resulted in a more ‘‘normal’’ bond length of r C–N⫽1.1587 Å. The differences between the various structures are attributed to the presence of a flat bending potential in InCN. The same situation could Downloaded 31 Aug 2002 to 128.196.209.95. Redistribution subject to AIP license or copyright, see http://ojps.aip.org/jcpo/jcpcr.jsp J. Chem. Phys., Vol. 117, No. 10, 8 September 2002 (2) apply to ZnCN as well, in that the calculation of an r m geometry could yield a more typical C–N bond distance. However, this result would also imply a flat bending potential in ZnCN. An analysis of the vibrational structure suggests otherwise, as discussed. The shorter C–N bond distance may be a real effect. B. Preference for a linear cyanide structure The existence of a T-shaped geometry for NaCN and KCN has been explained by simple electronegativity arguments 共e.g., Refs. 6 – 8兲. Sodium and potassium donate their valence electron to the CN moiety, and an M⫹ CN⫺ polytopic structure results. More electronegative metals will have the tendency to keep their electrons and form more covalent linear isocyanide structures, and, at the far extreme, the most covalently bonded species will be the linear cyanides. For the 3d transition metal cyanides and their IIIA counterparts, such electronegativity arguments do not apply. Although copper and nickel are the most electronegative elements of this group, with values of 1.90 and 1.91, respectively,34 the next most electronegative element is gallium 共1.81兲. Zinc is considerably less electronegative than the others, with a value of 1.65—quite comparable to that of aluminum with 1.61. Yet, the most stable form of zinc, copper, and nickel is the linear cyanide species, while gallium and aluminum favor the isocyanide geometry. The explanation likely lies in how these elements bond to the CN group. Based on their electronic ground states (ZnCN:X 2 ⌺ ⫹ ;CuCN:X 1 ⌺ ⫹ ;NiCN:X 2 ⌬ i ), the bond to the CN moiety for these molecules is made through the (4s) orbital from the metal. A full 3d shell (3d 10) is still present on copper and zinc, and a 3d 8 shell on nickel. The 3d and 4s shells are still relatively close in energy.35 Hence, there is a possibility of metal– * backbonding of the 3d electrons into the empty * orbital on the CN moiety. The * orbital is composed predominantly of contributions from the p orbitals of the carbon atom, and consequently the metal forms the bond to this site, as opposed to nitrogen, creating the cyanide species. In both aluminum and gallium, the bond to the CN group occurs via a 3p or 4p 共兲 orbital. Aluminum has no 3d electrons for backbonding; the 3d orbitals on gallium have dropped considerably in energy relative to the 4p orbital, as opposed to the 4s, making backbonding to the CN group very unlikely. Because of the lack of * backbonding, there is no reason for gallium or aluminum to bond to the carbon. The more electropositive metal would rather bond to the more electronegative nitrogen atom of the C␦ ⫹ N␦ ⫺ functional group. It should also be mentioned that iron is most stable in the isocyanide form, FeNC.11 Iron has a 3d 6 configuration—two d electrons less than nickel. It may be that there is some critical number of d electrons that must participate in backbonding to produce the cyanide structure, as opposed to the isocyanide. Spectroscopy of such molecules as MnNC/ MnCN, CrNC/CrCN, etc., would certainly verify this hypothesis. It would also be of interest to establish the preferred structure of cobalt and the cyanide group. Millimeter-wave studies of ZnCN 4859 VI. CONCLUSION The measurement of the pure rotational spectrum of ZnCN and several of its isotopomers has demonstrated that the radical has a 2 ⌺ ⫹ ground electronic state 共a linear structure兲, and that there is a preference for zinc to bond to the carbon as opposed to the nitrogen atom. Therefore, zinc has similar bonding properties to other late 3d transition metals such as copper and nickel. Analysis of the vibrational satellite lines of the main isotopomer, 64ZnCN, indicate that the molecule is fairly rigid, and does not appear to undergo large-amplitude bending motions. However, estimates of the bending and heavy atom-stretching mode frequencies, relative to those of CuCN and NiCN, suggest it is not as tightly bound as these latter species. The metal–carbon bond length successively increases in going from CuCN to ZnCN to GaCN; the C–N bond distance, on the other hand, appears anomalously short 共⬃1.14 Å兲 in zinc cyanide, relative to the other two species, but is comparable to that found in InCN, (1) structure calculation. The formation of ZnCN, as using a r m opposed to ZnNC, can be attributed to metal– * backbonding of the 3d electrons. This bonding scheme is also possible for copper and nickel, but not for aluminum and gallium, which both favor the isocyanide geometry. ACKNOWLEDGMENTS This research is supported by National Science Foundation 共NSF兲 Grant Nos. CHE 98-17707 and AST 98-20576 and NASA Grant No. NAG5-10333. 1 J. J. Van Vaals, W. L. Meerts, and A. Dymanus, Chem. Phys. 86, 147 共1984兲. 2 T. Törring, J. P. Bekooy, W. L. Meerts, J. Hoeft, E. Tiemann, and A. Dymanus, J. Chem. Phys. 73, 4875 共1980兲. 3 K. Kawaguchi, E. Kagi, T. Hirano, S. Takano, and S. Saito, Astrophys. J. Lett. 406, L39 共1993兲. 4 J. S. Robinson, A. 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