Chemical Physics Letters 365 (2002) 514–524 www.elsevier.com/locate/cplett ~ 1A0): The millimeter/submillimeter spectrum of LiSH (X further investigations of the metal–sulfur bond A. Janczyk, L.M. Ziurys * Department of Chemistry and Department of Astronomy, Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA Received 28 June 2002; in final form 29 August 2002 Abstract The pure rotational spectrum of LiSH and its 6 Li and deuterium isotopomers has been recorded in the region 73–521 GHz using millimeter/sub-millimeter direct absorption techniques. These species were created by the reaction of H2 S or D2 S and lithium vapor in a dc discharge. Extensive Ka ladder structure was observed for all three isotopomers, indi~ 1 A0 electronic state. Rotational parameters have been decating that LiSH is a near-prolate asymmetric top with a X termined for the three species, enabling the calculation of a rmð1Þ structure. The Li–S–H bond angle was found to be 93°, indicating a high degree of covalent bonding in this molecule. Ó 2002 Elsevier Science B.V. All rights reserved. 1. Introduction While metal oxides and hydroxides species have been studied extensively by a variety of spectroscopic methods [1–6], many of their sulfide analogs in comparison have been neglected. Although metal–oxygen bonds are quite common in multiple areas such as combustion, corrosive processes and chemical vapor deposition [7,8], metal-sulfide bonds also play a relevant chemical role. For example, they are significant in biological systems in the structures of amino acids and proteins [9]. They additionally are important in such applications as catalysis, pollution control, and in me- * Corresponding author. Fax: +520-621-1532. E-mail address: [email protected] (L.M. Ziurys). chanical lubricants [10]. It is therefore of interest to study metal–sulfur bonds and determine their properties, in particular in relationship to their oxygen counterparts. One interesting class of molecules containing a metal–sulfur bond is the hydrosulfides, with the structure MSH. These species are thought to be particularly important because they serve as models for organic thiols MSR [11]. Also, many MOH compounds have been investigated spectroscopically, including those where M is an alkali metal [2,12], an alkaline earth element [1,13,14], a transition metal [4], and aluminum [3]. Hence, a good comparison can be made between the metal hydroxides and hydrosulfides. Metal hydroxide compounds in themselves exhibit interesting bonding and corresponding structural trends. For example, most metal hydroxides 0009-2614/02/$ - see front matter Ó 2002 Elsevier Science B.V. All rights reserved. PII: S 0 0 0 9 - 2 6 1 4 ( 0 2 ) 0 1 5 0 4 - X A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 are linear species such as CaOH, SrOH, BaOH and AlOH [1,3,14]. These molecules are thought to be highly ionic. In contrast, CuOH and AgOH are bent species, and are speculated to have a greater degree of covalency [4]. In between lie MgOH, NaOH and LiOH, which appear to be quasi-linear molecules with very low barriers to the bending motion [2,12,13]. In fact, calculations have shown that LiOH has virtually no barrier to a bent geometry up to an angle of 90° [12]. The sulfur analogs of these compounds that thus far have been investigated, on the other hand, have all proven to be bent. These species include the alkaline earth radicals MgSH [15], CaSH [16,17], SrSH [18,19], as well as NaSH [20]. Optical and pure rotational data have conclusively shown that these molecules are near-prolate asymmetric tops with M–S–H angle near 90°. Hence, they closely resemble H2 S. Therefore, the metal hydrosulfides appear to exhibit a greater degree of covalent bonding than their hydroxides analogs. Clearly, it would be of interest to investigate other metal hydrosulfide species to determine whether their structures are bent, linear, or even quasi-linear, and examine any geometrical trends. LiSH is one possible candidate in this respect. A study of the lithium form of the hydrosulfides is of particular relevance because this species can be most directly compared to H2 S. Moreover, lithium-alkyl compounds are extremely well known in organic synthesis; there has been much speculation concerning the nature of the Li–R bond [21,22], which has been consequently extended to Li–SR systems [11]. Quantum calculations have also been carried out for LiSH by several authors. The earliest study was by Pappas [11], who suggested that the molecule is bent with a Li–S–H angle of 97°, and with a Li–S bond length that is 0.05 A greater than that found experimentally in the LiS radical [23]. More recent computations by Remko and Rode [24] and Magnusson [25] also indicate a bent geometry, with an angle near 94° and 91°, respectively. A crystal structure of LiSH has been published as well [26]. As a continuation of our work on metal–ligand interactions, we have recorded the pure rotational ~ 1 A0 ground electronic spectrum of LiSH in its X state. To our knowledge, this work is the first gas- 515 phase spectroscopic investigation of this species in its monomeric form. The spectrum of this molecule was measured using millimeter/sub-mm direct absorption techniques and those of LiSD and 6 LiSH were recorded as well. LiSH is unstable under ordinary conditions, and rapidly hydrolyses in air [11]. Hence, it had to be created in a dc discharge. Here we present our measurements and analysis, and discuss bonding in metal hydrosulfides based on these new data. 2. Experimental The rotational spectrum of LiSH and two of its isotopomers were measured using one of the millimeter-wave spectrometers of the Ziurys group, which is described in detail elsewhere [27]. Briefly, the source of radiation consists of a phase-locked Gunn oscillator combined with a multiplier, which enable frequency coverage of 65–640 GHz. The microwave radiation is propagated quasi-optically through the cell, a double pass system, using a series of Teflon lenses, a wire grid, and a rooftop reflector. The radiation is then detected by a helium cooled, InSb hot electron bolometer. LiSH was created by the reaction of lithium vapor and H2 S in a dc discharge. The metal vapor was generated by placing solid lithium in a metal– lined alumina crucible and heating it in a Broidatype oven. The metal liner was necessary to prevent the molten lithium from attacking the crucible. The Li vapor was then reacted with about 4 mTorr of H2 S, introduced through a tube over the top of the oven. Approximately 20 mTorr of argon, which was added through the bottom of the oven, was used as a carrier gas for the lithium. The optimum discharge current was 0.21 A at 70 V. Discharging the reaction mixture resulted in bright pink emission whose intensity depended upon the concentration of lithium vapor. To create LiSD, D2 S (Cambridge Laboratory) was reacted instead of H2 S. To preferentially synthesize the 6 Li isotopomer, enriched lithium-6 metal (Aldrich) was used. After the initial search using data scans successively covering 100 MHz in range (see Section 3), actual transition frequencies were determined 516 A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 from 5 MHz scans, which were always recorded in pairs, increasing and decreasing in frequency. Usually only one such pair was needed to obtain a sufficient signal-to-noise ratio. However, for the weaker Ka components, as many as 8 pairs were averaged. The center frequency of all features was determined by fitting a Gaussian curve to the line profile. 3. Results To initially search for the spectrum of LiSH, a geometry had to be predicted. Because NaSH [20], MgSH [16] and CaSH [17] are all bent species, the lithium analog was likely to have a similar structure and a 1 A0 ground electronic state. The Li–S bond length was assumed to be that of the dia tomic species, LiS [23], which was rLi–S ¼ 2:164 A (r0 ); for the S–H or (S–D) bond distance, that of : [20]). NaSH (or NaSD) was used (rS–H ¼ 1:396 A The bond angle was chosen to be that of H2 S (92°: [28]), because LiSH probably most closely resembles this molecule of all the alkali hydrosulfides. From the geometric parameters, A, B, and C rotational constants were calculated. The major centrifugal distortion constants, DJ and DJK , were estimated by mass-scaling those of NaSH and NaSD. Using those five spectroscopic parameters, rotational frequencies were predicted for all three isotopomers, assuming a-type transitions (DKa ¼ 0, DKc ¼ 1); a-type lines have been routinely observed for the other metal hydrosulfides [15,17,19]. The predicted transition frequencies in the end turned out to be very close to those actually measured. (Only later were the ab initio calculations found in the literature [11,24,25].) Hence, for the main LiSH isotopomer, a group of lines resembling an a-type pattern was initially found within a few GHz (2 GHz) of the predictions, and then a second transition was discovered. The Ka ¼ 0 component and the Ka ¼ 1 asymmetry doublets in both transitions were assigned initially on the basis of their stronger intensity and their position in frequency space relative to other observed lines. With two transitions observed, additional ones could be accurately predicted and were subsequently recorded. Assignment of additional Ka components was done by first finding the Ka ¼ 3 lines, identified because of their small asymmetry splitting which totally collapsed at lower J. With the Ka ¼ 0, 1 and 3 lines assigned, it was then relatively easy to predict and identify the Ka ¼ 2 asymmetry doublets and the Ka P 4 components, which were collapsed into single features. A similar situation occurred in the case of LiSD, where predictions were initially good enough to come within 7 GHz of the actual transition frequencies. The Ka ¼ 0 and Ka ¼ 1 lines were located because of their larger intensities, and the Ka ¼ 3 doublets were found because of their small asymmetry splitting. For the 6 Li isotopomer, Fig. 1. A stick figure showing the progression and relative intensities of the Ka components of the J ¼ 6 ! 7 transition of LiSH, LiSD and 6 LiSH. These patterns all clearly indicate that lithium hydrosulfide is a bent molecule. The patterns are similar for LiSH and 6 LiSH, with Ka ¼ 0 component located roughly in between the Ka ¼ 1 asymmetry doublets. In contrast, the Ka ¼ 0 line in LiSD is shifted to the left of the Ka ¼ 1 centroid, with other Ka components lying to the right at higher frequency. A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 candidate transitions were first identified in the spectrum of 7 LiSH, based on the natural lithium isotope abundances, and then searched for with lithium-6 enriched metal. Actual lines arising from 6 LiSH then naturally appeared more intense. The Ka asymmetry pattern was very easily assigned because it closely mimicked that of 7 LiSH. These variations in patterns are shown in Fig. 1, which displays stick spectra of the J ¼ 6 ! 7 transition of all three isotopomers. The 7 LiSH and 6 LiSH patterns are very similar: the Ka ¼ 0 line is located near the centroid of Ka ¼ 1 asymmetry doublets, the Ka ¼ 2 doublets are split by 200 MHz near the Ka ¼ 0 feature, and the rest of the components are collapsed into single features and located at lower frequency. In contrast, for LiSD, the Ka ¼ 2, 3 and 4 components are located to higher frequency relative to the Ka ¼ 0 line, and the asymmetry doublets for Ka ¼ 2 and 3 have significantly larger splittings. These effects are expected, as LiSD is more asymmetric. In general, these observed patterns clearly indicate a bent molecule of the Cs point group. Representative spectra are shown in Figs. 2 and 3. A section of the J ¼ 6 ! 7 transition of the Fig. 2. Spectrum of a section of the J ¼ 6 ! 7 rotational ~ 1 A0 ) near 256 GHz, showing the Ka ¼ 0 transition of LiSH (X and Ka ¼ 2 through 5 components. At this frequency, only the Ka ¼ 2 lines are split because of asymmetry doubling, as illustrated in the spectrum. The lines marked by asterisks are unidentified. This spectrum is a composite of 30, 100 MHz scans, each lasting 1 min in duration. 517 main lithium isotopomer near 256 GHz is presented in Fig. 2. The quantum number designation is (Ka00 ; Kc00 )–(Ka0 ; Kc0 ). The Ka ¼ 0, 2, 3, 4 and 5 components are visible in these data; only the Ka ¼ 2 lines are split by asymmetry doubling. The features follow the progression of a-type transitions of near-prolate asymmetric top with Cs symmetry. Asterisks indicate unidentified lines. In Fig. 3, spectra of a section of the J ¼ 7 ! 8 transitions of both LiSD and 6 LiSH near 281 and 331 GHz, respectively, are displayed. The upper panel shows the data for the deuterium isotope over a 1.5 GHz range, and includes the Ka ¼ 0, 4, Fig. 3. Spectra of a section of the J ¼ 7 ! 8 rotational transitions of LiSD and 6 LiSH near 281 and 331.5 GHz, respectively. In the LiSD spectrum (top panel), the Ka ¼ 4 and 5 asymmetry doublets are collapsed and appear to the higher frequency side of the Ka ¼ 0 line. For 6 LiSH, only the Ka ¼ 0 and 2 components are visible, the latter which are split by asymmetry by over 600 MHz. The other Ka components are located to lower frequency of the Ka ¼ 0 line. Unidentified features are indicated by asterisks. The LiSD spectrum is a composite of 15, 100 MHz scans, each lasting about 1 min in duration, and the 6 LiSH data are a composite of 10 similar scans. 518 Table 1 ~ 1 A0 Þa Selected observed rotational transitions of LiSH, LiSD, and 6 LiSHðX 2 3 3 3 7 7 7 7 7 7 7 7 7 7 7 7 7 8 8 8 8 8 8 8 8 8 8 8 8 8 8 8 9 Ka0 0 1 0 1 1 6 6 5 5 4 4 3 3 2 0 2 1 1 7 7 6 6 5 5 4 4 3 3 2 0 2 1 8 Kc0 2 3 3 2 7 1 2 3 2 4 3 4 5 6 7 5 6 8 1 2 2 3 3 4 5 4 5 6 7 8 6 7 2 J 00 1 2 2 2 6 6 6 6 6 6 6 6 6 6 6 6 6 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 8 Ka00 0 1 0 1 1 6 6 5 5 4 4 3 3 2 0 2 1 1 7 7 6 6 5 5 4 4 3 3 2 0 2 1 8 Kc00 1 2 2 1 6 0 1 2 1 3 2 3 4 5 6 4 5 7 0 1 1 2 2 3 4 3 4 5 6 7 5 6 1 LiSH 6 LiSD mobs mobs mcalc 73286.203 107986.018 109913.610 111801.081 251836.709 253580.778 253580.778 254439.925 254439.925 255156.006 255156.006 255729.134b 255729.134b 256063.948 256172.532 256304.105 260723.499 287757.665 288635.854 288635.854 289775.726 289775.726 290757.602 290757.602 291577.204 291577.204 292236.822b 292236.822b 292594.111 292643.520 292954.113 297907.022 323224.830 )0.005 0.006 )0.005 )0.058 )0.014 0.030 0.030 0.012 0.012 )0.033 )0.034 – – 0.000 0.017 )0.072 0.005 )0.013 0.043 0.043 0.012 0.012 0.001 0.001 )0.043 )0.047 – – )0.010 0.021 )0.040 0.016 0.006 LiSH mobs mobs mcalc mobs mobs mcalc 239412.422 245227.331 245227.331 245977.302 245977.302 246619.098 246619.098 247195.987 247170.448 247089.235 246041.160 248596.840 254862.750 273461.548 279257.257 279257.257 280248.091 280248.091 281111.120 281111.120 281857.407b 281857.407b 282559.131 282507.928 282268.286 280627.804 284515.280 291086.417 )0.033 )0.026 )0.026 0.015 0.015 0.060 )0.087 )0.056 0.027 0.048 )0.007 )0.056 0.006 0.011 )0.004 )0.004 0.013 0.013 )0.016 )0.015 – – 0.014 0.017 0.032 0.010 )0.050 0.018 284478.348 286762.674 286762.674 287854.787 287854.787 288767.666 288767.666 289503.386 289502.161 289903.395 289960.028 290300.950 295859.277 325040.196 326245.774 326245.774 327691.669 327691.669 328939.976 328939.976 329985.486 329985.486 330835.011 330831.012 331249.353 331190.770 331845.049 338036.154 0.011 )0.024 )0.024 0.041 0.041 0.014 0.022 )0.163 0.092 0.040 0.019 )0.077 0.025 0.016 0.006 0.006 )0.017 )0.017 0.025 0.025 0.008 0.016 0.116 )0.123 0.031 )0.022 )0.029 0.0131 A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 J0 8 1 7 7 6 6 5 5 4 4 3 3 0 2 2 1 8 8 1 7 7 6 6 5 5 4 4 3 3 0 2 2 1 8 8 1 7 7 6 6 5 1 9 3 2 4 3 5 4 6 5 7 6 9 8 7 8 2 3 10 3 4 5 4 6 5 7 6 8 7 10 9 8 9 7 6 14 7 8 9 8 10 8 8 8 8 8 8 8 8 8 8 8 8 8 8 8 8 9 9 9 9 9 9 9 9 9 9 9 9 9 9 9 9 9 13 13 13 13 13 13 13 13 8 1 7 7 6 6 5 5 4 4 3 3 0 2 2 1 8 8 1 7 7 6 6 5 5 4 4 3 3 0 2 2 1 8 8 1 7 7 6 6 5 0 8 2 1 3 2 4 3 5 4 6 5 8 7 6 7 1 2 9 2 3 4 3 5 4 6 5 7 6 9 8 7 8 6 5 13 6 7 8 7 9 323224.830 323656.553 324676.775 324676.775 325958.314 325958.314 327062.907 327062.907 327986.554 327986.554 328732.072 328735.745 329064.771 329104.143 329617.887 335065.303 359092.465 359092.465 359530.696 360704.068 360704.068 362126.978 362126.978 363354.308 363354.308 364382.526 364382.526 365216.544 365223.082 365430.319 365591.476 366296.906 372195.109 502401.524 502401.524 502728.693 504646.346 504646.346 506631.291 506631.291 508349.534 0.006 0.012 0.014 0.014 )0.006 )0.006 )0.017 )0.017 )0.025 )0.036 0.126 )0.175 0.025 )0.004 )0.003 0.016 0.001 0.001 0.021 )0.014 )0.014 )0.030 )0.030 )0.021 )0.021 )0.015 )0.038 0.113 )0.158 0.020 )0.037 0.044 0.021 0.020 0.020 )0.022 0.025 0.025 )0.012 )0.012 )0.009 307453.542 314145.762 314145.762 315264.119 315264.119 316242.694 316242.694 317098.489b 317098.489b 317852.372 317946.243 315004.601 317399.708 320580.486 327231.694 0.018 0.008 0.008 0.025 0.025 0.021 0.016 – – )0.035 0.065 0.002 0.025 0.005 )0.008 341383.668 349027.651 349027.651 350274.800 350274.800 351371.608 351371.608 352342.435b 352342.992b 353202.277 353362.982 349159.020 352477.604 356796.934 363286.194 )0.005 )0.004 )0.004 )0.014 )0.014 )0.004 )0.017 – – )0.126 0.096 )0.011 )0.022 0.029 )0.012 365571.278 366980.201 366980.201 368605.782 368605.782 370010.423 370010.423 371189.418 371189.418 372148.005 372156.501 372345.435 372567.767 373417.480 380177.212 0.014 0.012 0.012 )0.043 )0.043 0.035 0.035 0.017 )0.002 0.012 )0.048 )0.017 )0.043 0.053 0.005 A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 9 9 9 9 9 9 9 9 9 9 9 9 9 9 9 9 10 10 10 10 10 10 10 10 10 10 10 10 10 10 10 10 10 14 14 14 14 14 14 14 14 519 A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 and 5 components, as well as unidentified features marked by asterisks. As the figure illustrates, the asymmetry doubling is completely collapsed in the Ka ¼ 4 and 5 lines. In the lower panel, which covers approximately 1 GHz in frequency, the Ka ¼ 0 and 2 components of 6 LiSH are visible. Here the Ka ¼ 2 lines are split by over 0.5 GHz due to the asymmetry effects. A subset of the data measured for these three species are presented in Table 1. (For the complete data set, please contact the authors.) Altogether, almost every Ka component (Ka 6 8) of 12 individual rotational transitions was recorded for 7 LiSH in frequency range 73–521 GHz, a total of 104 individual spectral lines. For LiSD, all components with Ka 6 7 were recorded for four transitions, and for 6 LiSH, a similar range of Ka features were measured for three transitions. The lowest transition measured for 7 LiSH was for J ¼ 1 ! 2; although 7 Li has a nuclear spin of I ¼ 3=2, no evidence of quadrupole hyperfine interactions were found in the single line recorded. mobs b In MHz, for m ¼ 0. For the complete data set, contact L.M. Ziurys. Blended lines. 4. Analysis a 5 4 4 0 3 3 2 2 1 9 11 10 14 12 11 13 12 13 13 13 13 13 13 13 13 13 13 5 4 4 0 3 3 2 2 1 8 10 9 13 11 10 12 11 12 508349.534 509802.621 509802.941 510222.581 511004.972 511042.547 511264.227 513188.518 520363.252 )0.009 )0.036 0.025 )0.034 )0.064 0.033 0.027 )0.020 )0.008 mobs mobs 14 14 14 14 14 14 14 14 14 Kc0 Ka0 J0 Table 1 (continued) J 00 Ka00 Kc00 LiSH mobs mcalc LiSD mobs mcalc 6 LiSH mobs mcalc 520 All three data sets were analyzed using a S-reduced Hamiltonian that consisted of terms for molecular frame rotation and its centrifugal distortion [29]. The Hamiltonian was incorporated into the non-linear least-squares code, SPFIT, developed by Pickett [30]. The data were analyzed by first fitting only the lower Ka components of each species (Ka ¼ 0, 1 and 3). Spectral lines that were partially blended (usually Ka ¼ 3 and 4 asymmetry doublets) were not included in the fit. This analysis produced a preliminary set of constants. Then additional Ka components were subsequently included in the fit, which required increasingly higher centrifugal distortion corrections. In the final fit for 7 LiSH, 12 such parameters were found necessary to obtain a reasonable rms, which is 62 kHz, as shown in Table 2. These constants included four sixth-order terms (HJJK , HJKK , h2 , h3 ), three eighth-order corrections (LJJK , LJK , LKKJ ) and one 10th-order term (PKJ ). Use of such high order constants is justified, given that components as high as Ka ¼ 8 were included in the A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 521 Table 2 Rotational constants for LiSH, 6 LiSH and LiSDa A B C DJ DJK d1 d2 HJJK HJKK h2 h3 LJJK LJK LKKJ l3 PKJ rms of fit a LiSH LiSD 6 293283(17) 18959.3604(92) 17687.1945(89) 0.077746(11) 5.83133(80) )0.006309(16) )0.002428(30) 0.0002416(25) 0.004626(55) 2:8ð1:2Þ 107 3:2ð2:7Þ 108 1:48ð61Þ 108 2:90ð24Þ 107 1:21ð14Þ 105 151540.6(4.4) 18797.388(29) 16582.180(26) 0.065721(61) 4.9052(16) )0.011131(78) )0.006615(25) 0.0002489(94) 0.002522(55) 293407(41) 21565.078(44) 19935.302(42) 0.09804(14) 7.4396(23) )0.00919(15) )0.003898(36) 0.000354(16) 0.006358(70) LiSH 1:18ð22Þ 105 3:2ð1:1Þ 108 0.062 3:4ð2:1Þ 107 2:49ð66Þ 106 5:3ð3:9Þ 107 1:258ð77Þ 105 1:10ð22Þ 107 0.036 0.053 In MHz. analysis, and given the range of rotational quantum number (J ¼ 1 to J ¼ 13), which encompassed transitions over a broad frequency range (73–521 GHz). Furthermore, a similar set of constants has been used to successfully fit the millimeter-wave spectrum of SrSH [19], which included a comparable data set. For LiSD and 6 LiSH, fewer higher order centrifugal distortion parameters were required to achieve a rms of 36 and 53 kHz, respectively (see Table 2). These data sets were considerably smaller. When the partially blended features were included in the fit, the values of rms increased to 122, 167 and 53 kHz for 7 LiSH, LiSD and 6 LiSH. Two types of structures for LiSH were determined from the rotational constants in Table 2: r0 and rmð1Þ . While a r0 geometry is clearly inferior because it does not compensate for zero- point vibrations, such a calculation was carried out nevertheless for comparison with other molecules. Because three moments of inertia were experimentally established for each isotopomer, there are nine separate moments for which to determine three geometric parameters (rS–H , rLi–S and hLi–S–H ). A least squares fit to all nine values yielded , rS–H ¼ 1:353 A and hLi–S–H ¼ rLi–S ¼ 2:146 A 93:0°, as shown in Table 3. (Fitting two moments of inertia in the three separate combinations of pairs, and then taking the average, gave virtually identical results for the structure.) In contrast, a rmð1Þ structure attempts to account for at least some of the contribution of the vibrational motion to Table 3 ~ 1 A0 ) Structures for LiSH (X rLiS ) (A rSH ) (A hLi–S–H (deg.) Experimental r0 rmð1Þ 2.146 2.143 1.353 1.348 93.0 93.2 Theoretical re 2.145a , 2.149b 1.340a , 1.351b 91.4a , 94.6b a b From [25]. From [24]. 522 A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 Table 4 Comparison of structures (r0 ) for alkali and alkaline earth hydrosulfides M–SH rM–S ) (A LiSH NaSHa MgSH CaSH SrSHa 2.146 2.479 2.316 2.564 2.706 a b (1) (1) (15) (6) (3) rS–H ) (A hM–S–H (deg.) References 1.353 (1) 1.354 (1) 1.339b 1.357 (5) 1.358 (4) 93.0 (1) 93.1 (1) 87 (20) 91 (5) 91.04 (3) This work [20] [15] [17] [19] Structure refit; see text. Held fixed. the equilibrium geometry by introducing a correction term proportional to the square root of the 1=2 moment of inertia, ðI a Þ [31] 1=2 I0a ¼ Ima þ ca Ima : ð1Þ Here I0a refers to the moments of inertia related to the r0 structure, Ima the corrected moments, and ca is a correct factor determined from fitting the data. A linear least-squares fit to the moments of inertia for all three isotopomers resulted in a geometry very similar to the r0 structure, namely rLi–S ¼ , rS–H ¼ 1:348 A and hLi–S–H ¼ 93:2°. These 2:143 A values are also given in Table 3. (The pffiffiffiffiffiffiffiffiffi ffi correction and cðcÞ ¼ factorspffiffiffiffiffiffiffiffiffi wereffi cðaÞ ¼ 0:0321 amu A ). 0:0311 amu A 5. Discussion This study of the pure rotational spectrum of LiSH has established that this molecule is indeed bent, with an angle of 93° – very close to that of H2 S (92.1°). A bent geometry was also predicted by theory [11,24,25], but two of the three calculated angles were noticeably larger than the experimental values (97° and 94.6°). On the other hand, the structures obtained by both Remko and Rode [24] and Magnusson [25] are still reasonably close to those determined experimentally, as shown in Table 3. Because the bond angle in LiSH is so close to that of H2 S, it is quite likely that the bonding in the hydrosulfide is predominantly covalent. Pappas [11], in fact predicts the Li–S bond is covalent, based on Mulliken populations, but then argues against this conclusion, suggesting strictly an ionic interaction. Magnusson [25] also attributes the bend geometry to the effects of covalency. If LiSH were strictly an ionic molecule, it should have a linear structure in analogy to LiOH and the alkaline earth hydroxides [12,14]. In fact, this linear geometry is expected if ion-dipole interactions dominate the bonding, a situation where the molecule can be viewed at as a metal cation interacting with a negative ligand (OH or SH ) [25]. Clearly, metal hydrosulfides prefer the bent geometry, probably a result of bonding via p2 orbitals. A fair degree of covalent character must exist in the Li–S bond and the other metal–sulfur bonds to produce such structures. This property distinguishes LiSH from LiOH, which is on average, linear [12]. LiSH could also be exceptionally ÔfloppyÕ and have a low barrier to opening to a linear form, in the opposite analogy to LiOH. Unfortunately, vibrational excited states of LiSH have not been observed in this work. However, some information about the rigidness of a molecule can be obtained from the inertial defect, D0 , which consists of a harmonic and Coriolis terms [32] D0 ¼ Dharm þ DCor 0 0 : ð2Þ The Coriolis term is thought to be small for simple molecules such that the major contribution to the inertial defect is Dharm . This term arises from vi0 brations that distort the structure of molecule. Hence, the magnitude of D0 reflects on the degree of Ôfloppiness.Õ Inertial defects calculated for LiSH, LiSD2 and 6 , reLiSH are 0.194, 0.257, and 0:193 amu A spectively. These values are relatively large, compared with other triatomic species [32]. Hence, A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 there is likely some vibrational distortion of the molecule. In comparison, the inertial defects for MgSH and 2 NaSH are D0 ¼ 0:158ð4Þ and [20]. The value for sodium hydro0:203 amu A sulfide is comparable to that of lithium, while the magnesium number is smaller. Because magnesium and sodium hydrosulfides are heavier molecules, it might be expected that their initial defects would be larger than their lithium counterpart, as has been found in studies of metal amide species [33]. The fact that they are not, is, again, suggestive that LiSH does not have a particularly rigid structure. If the major contribution to the inertial defect arises from the harmonic term, then the effective frequency of vibration which distorts the molecule, can be estimated. This approximation assumes that the vibrational frequencies that contribute to non-planarity can be replaced by an effective value, xeff . Then, according to Watson [32], the following relationship can be derived 2 xeff 3 h : hcD0 ð3Þ Using this formula, the effective vibrational frequency for LiSH was calculated to be xeff 521 cm1 , while that of LiSD is 390 cm1 . The geometry of LiSH can additionally be compared to those of NaSH and the alkaline earth hydrosulfides. The r0 structures for these compounds are all listed in Table 4. (The structure for NaSH was analyzed using the rotational constants from [20]. The SrSH geometry was recalculated using the data in [19].) There are some obvious trends in this data set. First of all, the metal–sulfur bond distance increases fairly uniformly with the size of the metal atom. Secondly, the sulfur–hydrogen bond lengths, when actually fit, have re. markably close values near 1:355 0:003 A Within the quoted errors, they are all essentially the same. In contrast, the hydrosulfide bond angles vary in the range 87°–93°. The angle for MgSH is smallest but has a large error; isotopic substitution was not carried out for this species, so the comparison is not as appropriate. The angles for SrSH and CaSH are better defined and are about 91°, while those of LiSH and NaSH are the same with the quoted uncertainty at a value of 93°. If these r0 523 structures are to be believed, then it appears that the alkaline-earth hydrosulfides have a slightly smaller bond angle than the alkali analogs. This effect likely arises from the presence of the unpaired electron on the alkaline earth species, which is thought to reside primarily on the metal atom [19]. This extra electron does not exist for the alkali hydrosulfides. Repulsion likely occurs between this unpaired electron and the two sets of lone pairs on the sulfur atom, resulting in a slight closing of the M–S–H angle relative to that in the alkali hydrosulfides. It would certainly be of interest to study such species as KSH and BaSH to see if this apparent difference between the alkali and alkaline-earth species continues down the periodic table. 6. Conclusion This millimeter-wave study of the pure rotational spectrum of LiSH has shown that indeed this molecule is bent in its ground electronic state, in contrast to its oxygen counterpart, LiOH, which is linear. The bond angle found in LiSH, from a rmð1Þ calculation, is 93.2° – quite close to the bond angle in H2 S. Substitution of a lithium atom in the place of hydrogen therefore did not significantly change the basic H2 S structure. Consequently, LiSH appears to be predominantly a covalently bonded molecule, in contrast to LiOH. This study is further evidence that metal-sulfide bonds do vary in their properties from metal–oxide bonds. Studying additional species containing such bonds would be useful in further elucidating metal–sulfur interactions. Acknowledgements This research is supported by NSF Grant CHE98-17707. References [1] C.R. Brazier, P.F. Bernath, J. Mol. Spectrosc. 114 (1985) 163. 524 A. Janczyk, L.M. Ziurys / Chemical Physics Letters 365 (2002) 514–524 [2] P. Kuijpers, T. T€ orring, A. Dymanus, Chem. Phys. 15 (1976) 457. [3] A.J. Apponi, W.L. Barclay, L.M. Ziurys, Astrophys. J. (Letters) 414 (1993) L129. [4] C.J. Whitham, H. Ozeki, S. Saito, J. Chem. Phys. 110 (1999) 11109. [5] K. Namiki, S. Saito, J. Chem. Phys. 107 (1997) 8848. [6] C. Yamada, E. Hirota, J. Chem. Phys. 111 (1999) 9587. [7] A.J. Bridgeman, J. Rothery, J. Chem. Soc., Dalton Trans. (2000) 211. [8] C.W. Bauschlicher, P. Maitre, Theor. Chim. Acta 90 (1995) 189. [9] M.K. Campbell, Biochemistry, Saunders College Publishing, Orlando, 1995. [10] I. Kretzschmar, D. Schr€ oder, H. Schwarz, P.B. Armentrout, Adv. Met. Semiconductor Clusters 5 (2001) 347. [11] J.A. Pappas, J. Am. Chem. Soc. 100 (1978) 6023. [12] A.J. Apponi, L.M. Ziurys, F.-M. Tao, K. Higgins, W. Klemperer, International Symposium on Molecular Spectroscopy (1996) paper WF01. [13] A.J. Apponi, M.A. Anderson, L.M. Ziurys, J. Chem. Phys. 111 (1999) 10919. [14] D.A. Fletcher, M.A. Anderson, W.L. Barclay Jr., L.M. Ziurys, J. Chem. Phys. 102 (1995) 4334. [15] A. Taleb-Bendiab, D. Chomiak, Chem. Phys. Lett. 334 (2001) 195. [16] C.N. Jarman, P.F. Bernath, J. Chem. Phys. 98 (1993) 6697. [17] A. Taleb-Bendiab, F. Scappini, T. Amano, J.K.G. Watson, J. Chem. Phys. 104 (1996) 7431. [18] W.T.M.L. Fernando, R.S. Ram, L.C. OÕBrien, P.F. Bernath, J. Phys. Chem. 95 (1991) 2665. [19] D.T. Halfen, A.J. Apponi, J.M. Thompsen, L.M. Ziurys, J. Chem. Phys. 115 (2001) 11131. [20] E. Kagi, K. Kawaguchi, Astrophys. J. (Letters) 491 (1997) L129. [21] A. Streitwieser Jr., J.E. Williams Jr., S. Alexandratos, J.M. McKelvey, J. Am. Chem. Soc. 98 (1976) 4778. [22] D.B. Grotjahn, A.J. Apponi, M.A. Brewster, J. Xin, L.M. Ziurys, Angew. Chem. Int. Ed. 37 (1998) 2678. [23] M.A. Brewster, L.M. Ziurys, Chem. Phys Lett. 349 (2001) 249. [24] M. Remko, B.M. Rode, J. Mol. Struct. (Theochem) 505 (2000) 269. [25] E. Magnusson, J. Phys. Chem. A 105 (2001) 3881. [26] H. Jacobs, R. Kirchgaessner, J. Bock, Z. Anorg. Allg. Chem. 569 (1989) 111. [27] L.M. Ziurys, W.L. Barclay Jr., M.A. Anderson, D.A. Fletcher, J.W. Lamb, Rev. Sci. Instrum. 65 (1994) 1517. [28] T.H. Edwards, N.K. Moncur, L.E. Snyder, J. Chem. Phys. 46 (1967) 2139. [29] J.K.G. Watson, in: J.R. During (Ed.), Vibrational Spectra and Structure, Elsevier, Amsterdam, 1977. [30] H.M. Pickett, J. Mol. Spectrosc. 148 (1991) 371. [31] J.K.G. Watson, A. Roytburg, W. Ulrich, J. Mol. Spectrosc. 196 (1999) 102. [32] J.K.G. Watson, J. Chem. Phys. 98 (1993) 5302. [33] P.M. Sheridan, L.M. Ziurys, Can. J. Phys. 79 (2001) 409.
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