Journal of Molecular Spectroscopy 234 (2005) 34–40 www.elsevier.com/locate/jms Velocity modulation spectroscopy of molecular ions I: The pure rotational spectrum of TiCl+ (X3Ur) D.T. Halfen, L.M. Ziurys * Departments of Chemistry and Astronomy, Arizona Radio Observatory, and Steward Observatory, University of Arizona, 933 N. Cherry Avenue, Tucson, AZ 85721, USA Received 14 May 2005; in revised form 22 July 2005 Available online 26 September 2005 Abstract The pure rotational spectrum of the TiCl+ ion in its X3Ur ground state has been measured in the frequency range 323–424 GHz, using a combination of direct absorption and velocity modulation techniques. The ion was created in an AC discharge of TiCl4 and argon. Ten, eleven, and nine rotational transitions were recorded for the 48Ti35Cl+, 48Ti37Cl+, and 46Ti35Cl+ isotopomers, respectively; fine structure splittings were resolved in every transition. The rotational fine structure pattern was irregular with the X = 4 component lying in between the X = 2 and 3 lines. This result is consistent with the presence of a nearby 3Dr state, which perturbs the X = 2 and 3 sub-levels, shifting their energies relative to the X = 4 component. The data for each isotopomer were analyzed in a global fit, and rotational and fine structure parameters were determined. The value of the spin–spin constant was comparable to that of the spin–orbit parameter, indicating a large second-order spin–orbit contribution to this interaction. The bond length established for TiCl+, r0 = 2.18879 (7) Å, is significantly shorter than that of TiCl, which has r0 = 2.26749 (4) Å. The shorter bond length likely results from a Ti2+Cl structure in the ion relative to the neutral, which is thought to be represented by a Ti+Cl configuration. The higher charge on the titanium atom shortens the bond. 2005 Elsevier Inc. All rights reserved. Keywords: Spectroscopy; Ions; Rotational 1. Introduction The technique of velocity modulation (VM) has traditionally been used only in optical and infrared ion spectroscopy (i.e., 600–17 000 cm1) [1,2]. However, it is not limited to these spectral regions and has recently been shown to work at much longer wavelengths. Stephenson and Saykally [3] have demonstrated that velocity modulation can be applied at terahertz frequencies, and Savage, Apponi, and Ziurys [4,5] extended the scope of VM to the millimeter/sub-millimeter regime. At the longer wavelengths, the VM technique is not quite as powerful as in the infrared, for example, because the lines are somewhat undermodulated [3,4]. Nevertheless, * Corresponding author. Fax: +1 520 621 1532. E-mail address: [email protected] (L.M. Ziurys). 0022-2852/$ - see front matter 2005 Elsevier Inc. All rights reserved. doi:10.1016/j.jms.2005.08.004 the ion selectivity of this method is still a major advantage in eliminating neutral signals [4]. The first molecule studied with the mm/sub-mm VM instrument in the Ziurys group was SH+ [5]. The measurement of the pure rotational spectrum of this openshell ion demonstrated the potential of the spectrometer system to preferentially detect such species. Naturally obtaining the rotational spectrum of other ionic species using this instrument is of interest, in particular metalcontaining compounds. One such ion is TiCl+. Titanium chloride cation has been the subject of various studies over the past 15 years. It was observed initially by Balfour and Chandrasekhar [6] in 1990, who measured P-branch bandheads from 559 to 564 nm and assigned the spectrum as a 3P–X3D transition. Following this work, Kaledin et al. [7] used ligand field theory (LFT) to calculate the electronic states of TiCl+. D.T. Halfen, L.M. Ziurys / Journal of Molecular Spectroscopy 234 (2005) 34–40 Their computations indicated that a 3Ur term was the ground state, and therefore these authors suggested that the transition observed by Balfour and Chandrasekhar was the [17.9]3Dr–X3Ur system. Kaledin and Heaven [8] subsequently confirmed this assignment experimentally using direct laser absorption methods, and determined preliminary spectroscopic constants for the 3D and ground 3U states, as well. At the same time, Focsa et al. [9] used laser absorption/velocity modulation techniques to also measure the [17.9]3Dr–X3Ur band of TiCl+ with 0.005 cm1 resolution, establishing effective rotational, spin–orbit, and spin–spin parameters for both states. These authors also suggested that the X = 4 spin–orbit component in the X3Ur state was perturbed relative to the other two X components. Kaledin and Heaven [10] then conducted further measurements of the [17.9]3Dr–X3Ur and [17.9]3Dr–(1)3Dr transitions with associated LFT calculations, which predicted nearby 3 R and 3P states. The most recent work is by Focsa et al. [11,12] and Focsa and Pinchemel [13]. In the Focsa et al. [11] study, the [17.9]3Dr–X3Ur (v = 0 and 1) and the [17.9]3Dr–A3Dr systems were measured. Here, the X = 2 and 3 ladders of TiCl+ in its X3Ur (v = 0 and 1) and A3Dr (v = 0) states were found to interact with each other, while the X = 4 sub-level (X3Ur) remained free of any perturbations [11]. An analysis combining the data of the X3Ur (v = 0 and 1) and A3Dr (v = 0) states was then performed to establish ‘‘deperturbed’’ spectroscopic constants for these states [11]. Focsa et al. [12] additionally performed density functional theory (DFT) and LFT calculations on TiCl and TiCl+, and determined that the ionization potential of titanium chloride was 7.06 eV. In this study, we report the first measurement of the pure rotational spectrum of TiCl+ in its X3Ur (v = 0) state. The ion was synthesized in an AC discharge of TiCl4. All three spin components were observed for the isotopomers 48Ti35Cl+, 48Ti37Cl+, and 46Ti35Cl+. This study was conducted using a combination of velocity modulation (for ion selectivity) and direct absorption (for sensitivity in scanning). Here, we present our results, spectral analysis, and a discussion of the data. 2. Experimental The pure rotational spectrum of TiCl+ was measured using the velocity modulation spectrometer of the Ziurys group, which has been described in detail elsewhere [4]. Briefly, the instrument consists of a radiation source, gas cell, and detector. Gunn oscillators/Schottky diode multipliers are used to generate frequencies between 65 and 650 GHz. The reaction chamber is a single-pass glass cell containing ring discharge electrodes, and a cooling jacket chilled to 65 C by methanol. The radiation is launched from a scalar feedhorn and is propagated 35 through the system quasi-optically using a series of Teflon lenses, two of which seal off the ends of the gas cell. The detector is an InSb hot electron bolometer, and the system is under computer control. Titanium chloride cation was created in an AC discharge of gas-phase TiCl4 and argon. The strongest signals of TiCl+ occurred using 20 mTorr of Ar and less than 1 mTorr of TiCl4; this mixture produced a bright blue–white plasma that dominated the normal purple discharge glow from the argon. The discharge was modulated at a rate of 20 kHz with a power level of 200 W at 600 X. Signals arising from TiCl+ were initially found by recording scans 100 MHz in coverage. First, scans were taken in source modulation mode with 2f detection for a higher signal-to-noise ratio. If lines were present, the data were then retaken in velocity modulation mode to select those signals arising from ions. Precise rest frequencies were obtained by averaging scans 5 MHz wide, taken in increasing and decreasing frequency, using source modulation. Typically, 1–4 scan pairs were needed to obtain a sufficient signal-to-noise ratio. Gaussian profiles were fit to the line shapes to obtain the center frequency and line width, which varied from 1.0 to 1.4 MHz from 323 to 424 GHz. The experimental accuracy is estimated to be ±40 kHz. 3. Results and analysis The transitions frequencies of 48Ti35Cl+ and Ti37Cl+ were initially predicted using the effective rotational parameters of Focsa et al. [9,11]. These constants were sufficiently accurate that signals from these ions were found within 100 MHz of the predictions. Previous estimates of rotational constants for 46Ti35Cl+ did not exist, so these were obtained from the 48Ti isotopomer by scaling by molecular mass. The observed rotational transitions of the three TiCl+ isotopomers are listed in Table 1. Ten, eleven, and nine transitions were measured for 48Ti35Cl+, 48Ti37Cl+, and 46 35 + Ti Cl , respectively. As shown in the table, each rotational transition is split into three fine structure components due to spin–orbit/spin–spin coupling and is labeled by the quantum number X. As is also evident in Table 1, the pattern of the spin–orbit splittings deviates considerably from a typical case (a) coupling scheme. For a given rotational transition, the X = 2 and 3 components are both shifted to significantly higher frequency as compared to the X = 4 line, such that the ordering of these features in increasing frequency is X = 2, 4, and 3, not X = 2, 3, and 4 as in a ‘‘normal’’ Ur state. This pattern can be seen in Fig. 1, which displays spectra of the J = 37 fi 38 transition of 48Ti35Cl+ near 395 GHz (top panel), and the J = 36 fi 37 transition of 46Ti35Cl+ near 392 GHz (bottom panel). These 48 36 D.T. Halfen, L.M. Ziurys / Journal of Molecular Spectroscopy 234 (2005) 34–40 Table 1 Observed rotational transitions of J00 fi J 0 X 30 fi 31 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 2 3 4 31 fi 32 32 fi 33 33 fi 34 34 fi 35 35 fi 36 36 fi 37 37 fi 38 38 fi 39 39 fi 40 40 fi 41 41 fi 42 a b 48 Ti35Cl+, 48 Ti37Cl+, and 46 Ti35Cl+ (X3Ur: v = 0)a 48 Ti35Cl+ 48 Ti37Cl+ mobs mobsmcalc 322927.414 323297.905 323156.037 333322.960 333705.663 333561.278 343716.434 344111.266 343964.669 354107.777 354514.788 354366.190 364496.962 364916.143 364765.753 374883.903 375315.282 375163.298 385268.555 385712.131 385558.767 395650.832 396106.617 395952.103 406030.676 406498.708 406343.266 416408.036 416888.324 416732.131 0.032 0.068 0.085 0.005 0.038 0.037 0.015 0.020 0.011 0.004 0.017 0.031 0.007 0.007 0.058 0.003 0.005 0.066 0.010 0.001 0.056 0.005 0.014 0.027 0.006 0.009 0.004 0.012 0.001 0.104 46 Ti35Cl+ mobsmcalc mobs 322953.671 323314.057 323171.257 333024.570 333396.685 333251.156 343093.350 343476.429 343329.329 353160.158 353554.693 353405.545 363224.870 363630.856 363479.909 373287.393 373704.867 373552.337 383347.712 383776.673 383622.750 393405.736 393846.223 393691.112 403461.443 403913.422 403757.295 413514.731 413978.255 413821.346 423565.431 424040.610 423883.213 0.037 0.105 —b 0.043 —b 0.111 0.014 0.047 0.005 0.002 0.031 0.004 0.014 0.027 0.022 0.002 0.025 0.053 0.005 0.018 0.063 0.007 0.002 0.071 0.003 0.001 0.002 0.007 0.024 0.043 —b 0.019 0.061 mobsmcalc mobsmcalc 328815.478 329199.173 329056.267 339400.167 339796.364 339651.042 349982.690 350391.441 350244.185 360562.942 360984.439 360835.220 371141.161 371575.125 371424.259 381716.920 382163.551 382011.184 392290.326 392749.576 392596.013 402861.286 403333.176 403178.597 413429.697 413914.287 413758.893 0.017 0.043 0.051 0.013 0.003 —b 0.003 0.043 0.016 —b 0.005 0.021 0.016 0.020 0.038 0.008 0.001 0.009 0.000 0.007 0.011 0.011 0.001 0.046 0.012 0.020 —b In MHz. Blended lines, not included in fit. two isotopomers were observed in natural abundance of titanium (48Ti:46Ti = 73.7:7.4). There are two frequency breaks in each spectrum of about 300 and 150 MHz, respectively. The ratio of relative intensities of the spin–orbit components is X = 2:3:4 = 5:2.2:1, indicating Tspin–orbit=Tso 355 K. No hyperfine splittings arising from the chlorine nuclear spin of I = 3/2 are visible in these spectra, a general result for the whole data set. These lines persisted in velocity modulation mode, as demonstrated in Figs. 2 and 3, which distinguished them from neutral species, in particular TiCl. In Fig. 2, the exact same transition from Fig. 1 is shown, but in velocity modulation mode. The features now display a first derivative line shape, and the signal-to-noise ratio has decreased by about a factor of 4. The velocity-modulated lines are also narrower than those generated by source modulation by about a factor of 1.5. The de- crease in intensity and line width is due to undermodulation of the spectral lines. The loss in signal-to-noise, however, is countered by effective neutral suppression, as demonstrated in Fig. 3. These data display the X = 2 component in the J = 38 fi 39 transition of 46 35 + Ti Cl in source modulation (top panel) and velocity modulation (bottom panel) modes. In the source modulation spectrum, there are seven features, all within the estimated frequency range of the respective component of TiCl+. The same data taken using velocity modulation show only one feature, the TiCl+ transition in question. No lines originating in excited vibrational states of TiCl+ were observed in this work, as opposed to other chloride molecules studied in our group, such as CoCl [14] and MnCl [15], where several vibrational states were found. This result is probably because the VM cell, D.T. Halfen, L.M. Ziurys / Journal of Molecular Spectroscopy 234 (2005) 34–40 48 Ω=2 Ti35Cl+ (X3Φr): J = 37 48 38 Ω=2 37 Ti35Cl+ (X3Φr): J = 37 38 Velocity Modulation Ω=4 Ω=3 Ω=3 Ω=4 395.640 395.660 395.945 395.965 46 * Ω=2 396.095 Ti Cl (X Φr): J = 36 35 + 3 * 392.300 392.585 37 Ω=3 Ω=4 392.280 396.115 * 392.605 392.735 * 392.755 Frequency (GHz) Fig. 1. Laboratory spectra of the J = 37 fi 38 transition of 48Ti35Cl+ (X3Ur) near 395 GHz and the J = 36 fi 35 transition of 46Ti35Cl+ near 392 GHz recorded in source modulation mode. There are two frequency breaks in each spectrum to display the three spin–orbit components, which are plotted on the same intensity scale. The spin– orbit spacing is irregular with the X = 4 component lying between the X = 2 and 3 lines. Unknown features in the spectra are marked with an asterisk. The spectra were created from a composite of three single 110 MHz wide scans, each acquired in 70 s, and then cropped to each display a 40 MHz frequency range. which is methanol-cooled, produces colder molecules than those that were made using a Broida-type oven. For TiCl+, Tso 355 K, for example, while Tso 480 K for CoCl [14]. Also, the vibrational separation of TiCl+ is 700 K (485 cm1) [11], making population of higher vibrational levels difficult. The spectrum of TiCl+ was analyzed using an effective HundÕs case (a) Hamiltonian, including rotation, spin–orbit, and spin–spin constants and their respective centrifugal distortion corrections: ^ eff ¼ H ^ rot þ H ^ so þ H ^ ss . H ð1Þ For each isotopomer, all rotational data from the three spin–orbit components were analyzed simultaneously in a global fit. To fit these data, the spin–orbit constant A 395.640 395.660 395.945 395.965 Frequency (GHz) 396.095 396.115 Fig. 2. Spectrum of the J = 37 fi 38 transition of 48Ti35Cl+ near 395 GHz taken in velocity modulation mode. There are two frequency breaks in the spectra to accommodate the three spin–orbit components, which are plotted on the same scale. These data have the firstderivative line profile characteristic of velocity modulation spectra. The spectrum was created from a composite of three single 110 MHz wide scans, each acquired in 70 s, and then cropped to display a 40 MHz frequency range. The signal-to-noise ratio is about a factor of 4 less than in source modulation mode (see Fig. 1). was held fixed to the value of Focsa et al. [11], but the spin–spin parameter k was allowed to vary. Higher-order spin–orbit and spin–spin terms (AD, AH, kD, and kH) were found to be necessary to achieve a good fit. Because the error was found to be comparable to its value, kH was fixed in the final fit for all three species. The resulting spectroscopic parameters are listed in Table 2. The rms of the fits ranged from 23 to 41 kHz. For comparison, the constants determined by Focsa et al. [9,11] are also listed in Table 2 for 48Ti35Cl+ and 48 37 + Ti Cl . The rotational parameters for 48Ti35Cl+ from Focsa et al. [11] are in good agreement with those established in this work, although k and the higher-order spin–orbit and spin–spin constants are significantly different. However, the constants of Focsa et al. [11] were determined from a deperturbation analysis. Thus, their fine structure parameters are not directly comparable, as the analysis here made no correction for perturbations. Furthermore, the mm wave analysis included the additional higher-order terms AH and kH, which impacts the fit as well. The rotational constants of Focsa et al. [9] for 48Ti37Cl+ are also in reasonable agreement with those established in this work. Again, there are some differences because Focsa et al. [9] only used the X = 2 and 3 components in their analysis, while here all three spin sub-levels were considered. A more direct comparison of the optical and mm wave parameters is given in Table 3. Here, the effective rotational constants from both the millimeter-wave and the optical studies are listed. The agreement between the two sets of parameters is very good for both chlorine isotopomers of TiCl+. Differences in the global 38 D.T. Halfen, L.M. Ziurys / Journal of Molecular Spectroscopy 234 (2005) 34–40 46 fits therefore must arise from variations in the individual data sets, as previously described. Ti35Cl+ (Ω = 2) J = 38 39 4. Discussion Source Modulation Velocity Modulation 413.40 413.43 413.46 Frequency (GHz) Fig. 3. Spectrum of the J = 38 fi 39, X = 2 transition of 46Ti35Cl+ near 413 GHz taken in source modulation mode (top panel: secondderivative spectrum) and velocity modulation mode (bottom panel: first-derivative spectrum). The intensity scale of the VM spectrum is four times less than that of the source modulation spectrum. The source modulation spectrum displays various lines, which disappear in the velocity modulation data. These features arise from unwanted neutral species. The source modulation and velocity modulation data are an average of two and twelve 100 MHz wide scans, respectively, each 70 s in duration. Table 2 Spectroscopic constants for Parameter B D A AD AH k kD kH rms r0 (Å) a b c d 48 35 48 Ti35Cl+, Ti Cl 48 Ti37Cl+, and The r0 bond lengths were calculated from the rotational constants for all three isotopomers of TiCl+ and are listed in Table 2. The bond lengths of the three isotopomers are very similar, illustrating that the molecule closely follows the Born–Oppenheimer approximation. The average bond length of TiCl+ is + r0 = 2.18879 (7) Å. The bond length of TiCl is significantly shorter than that of neutral TiCl: r0 = 2.26749 (4) Å [16]—a difference of 0.079 Å. This decrease is probably due to the additional electrostatic attraction in the ion relative to the neutral species. According to Focsa, Bencheikh, and Pettersson [12], TiCl+ can be thought of as Ti2+Cl with an electron configuration of (core) 5p11d1, as opposed to Ti+Cl0. TiCl is best represented as Ti+Cl with (core)11r11d15p1. The additional charge on the titanium atom results in a stronger electrostatic attraction between the two atoms, shortening the internuclear distance. The difference is not likely to be a question of covalent-type bonding because the valence 1d, 5p, and 11r orbitals are essentially nonbonding, arising from the 3d electrons on titanium. In addition to the TiCl+ ion, the neutral TiCl (X4Ur) molecule was also observed in the AC discharge of TiCl4. The relative intensity of the neutral compared to the ion is shown in Fig. 4. Here, spectra of the J = 38 fi 39 transition of TiCl+ (top panel) and the J = 39.5 fi 40.5 transition of TiCl (bottom panel) are displayed on the same intensity scale. There are frequency breaks in both spectra to include all of the 46 Ti35Cl+ (X3Ur: v = 0)a + 48 Ti37Cl+ 46 Ti35Cl+ mm wave Opticalb mm wave Opticalc mm wave 5216.6676 (21) 0.00256353 (78) 19 00 000d 2.7834 (89) 6.308 (36) · 105 44 04 278 (5000) 18.071 (46) 1.000 · 105d 0.037 2.1888077 (4) 5226.07 (54) 0.002728 (45) 19 04 570 (80) 0.489 (54) 5054.1115 (23) 0.00241142 (79) 19 00 000d 2.6012 (94) 5.647 (37) · 105 44 04 301 (5600) 16.993 (49) 5.992 · 106d 0.041 2.1887180 (5) 5056.12 (54) 0.00240 (11) 19 22 600 (90) 1.916 (18) 5311.9488 (17) 0.00265535 (69) 19 00 000d 2.8935 (70) 6.715 (35) · 105 44 04 291 (3900) 18.720 (37) 1.200 · 105d 0.023 2.1888587 (4) 11 030 (180) 0.507 (18) In MHz; errors are 3r in the last quoted digits. Deperturbed parameters from Focsa et al. [11]. From Focsa et al. [9]; based on X = 2 and 3 components only. Held fixed (see text). 47 157 (90) 0d D.T. Halfen, L.M. Ziurys / Journal of Molecular Spectroscopy 234 (2005) 34–40 39 Table 3 Effective rotational constants for the spin components of TiCl+a 48 Ti35Cl+ Parameter Beff (X = 2) Deff (X = 2) Beff (X = 3) Deff (X = 3) Beff (X = 4) Deff (X = 4) a b c 48 Ti37Cl+ b 46 Ti35Cl+ c mm wave Optical mm wave Optical mm wave 5213.6300 (43) 0.0026655 (17) 5219.5661 (43) 0.0026443 (17) 5216.7713 (43) 0.0023807 (17) 5213.75 (27) 0.002662 (54) 5219.72 (27) 0.002644 (45) 5217.26 (27) 0.002491 (54) 5051.2777 (43) 0.0025030 (16) 5056.8715 (42) 0.0024856 (14) 5054.1535 (43) 0.0022461 (15) 5050.27 (63) 0.002400 (90) 5056.09 (63) 0.002430 (90) 5053.7 (1.4) 0.00214 (45) 5308.7864 (52) 0.0027632 (20) 5314.9324 (50) 0.0027413 (20) 5312.0910 (67) 0.0024615 (27) In MHz; errors are 3r in the last quoted digits. From Focsa et al. [11]. From Focsa et al. [9]. 1.0 Ti35Cl+ (X3Φr): J = 38 48 Intensity (mV) Ω=2 0.5 Ω=4 39 Ω=3 * 0.0 -0.5 406.023 406.043 406.334 406.354 406.491 406.511 Ti35Cl (X4Φr): J = 39.5 40.5 1.0 Intensity (mV) Ω = 3/2 48 Ω = 5/2 Ω = 7/2 0.5 Ω = 9/2 0.0 -0.5 391.298 392.375 393.456 394.554 Frequency (GHz) Fig. 4. Spectrum of the J = 38 fi 39 transition of 48Ti35Cl+ near 406 GHz (top panel) and the spectrum of the J = 39.5 fi 40.5 transition of 48Ti35Cl near 391–394 GHz (bottom panel) taken in source modulation mode. There are two frequency breaks in the TiCl+ spectrum and three in the TiCl data, such that all spin–orbit components can be displayed. The data are plotted on the same scale given in mV. An unknown feature in the TiCl+ spectra is marked with an asterisk. The relative intensities of the ion and neutral species are virtually identical, illustrating the efficient production of TiCl+ in an AC discharge. Each of the spin component spectra is 40 MHz wide and were each extracted from a single 110 MHz scan, acquired in 70 s in source modulation mode. spin–orbit components for both molecules. As can be seen in the figure, the signal-to-noise ratio of TiCl+ is comparable to that of TiCl. Accounting for the number of spin–orbit components for both molecules, TiCl neutral is only 1.7 times stronger than the ion. This result is relatively unusual since ions are thought to make up a very small fraction of the species found in electrical discharges [4]. The relative strength of TiCl+ might be an indication that TiCl4 easily breaks apart into ions as well as neutral species in an AC discharge. Based on the relative intensities of the spin components, the spin–orbit temperature observed for TiCl is Tso 440 K, as compared to Tso 355 K for TiCl+—roughly similar. This result suggests that the neutral and the ion may both be made directly from TiCl4, rather than from secondary processes. The fine structure pattern in TiCl+ deviates considerably from that of pure case (a) with rotational transitions of the highest energy spin component, X = 4, appearing approximately midway in frequency between those originating in the two lower spin sub-levels. This rotational pattern is though to result from spin-electronic homogeneous perturbations, which follow the selection rules DX = 0, DK = DR = ±1, and DS = 0 [17]. As discussed by Focsa et al. [11], this perturbation is believed to arise from interactions with the nearby excited A3Dr state. This state lies 400 cm1 in energy above the X3Ur state and perturbs the X = 2 and 3 components, lowering their energies relative to the X = 4 sub-level. As a consequence, the regular case (a) spin–orbit pattern in TiCl+ is distorted. This perturbation manifests itself in the large value of k, 44 04 278 MHz, generated in the fit. In fact, for TiCl+, k > A, where A is the spin–orbit parameter. The k constant in part compensates for the shifting of the lower X ladders. In contrast, the ‘‘deperturbed’’ k value, estimated by Focsa et al. [11], is 11 030 MHz—over two orders of magnitude smaller. A large value of k was also found for the CoCl radical in its X3Ui state [14]. In this species, the X = 3 ladder was perturbed such that the spin–orbit components in a given rotational transition did not follow a regular case (a) pattern. The rotational data for CoCl, however, was easier to analyze because the perturbation only occurred in the X = 3 sub-level where k, but not A, is present in the diagonal matrix element. For TiCl+, the X = 2 level is additionally shifted, and both A and k enter into the its diagonal matrix element as competing parameters. 40 D.T. Halfen, L.M. Ziurys / Journal of Molecular Spectroscopy 234 (2005) 34–40 5. Conclusion References The pure rotational spectrum of TiCl+ in its X3Ur ground state has been recorded for the first time. The study of this ion has been aided by using velocity modulation techniques, which have been extended to millimeter/ sub-millimeter wavelengths. Curiously, in an AC discharge, signals generated for TiCl+ are nearly equivalent to those of the neutral TiCl, indicating that this ion production method can be very efficient for certain species. Previous measurements of several electronic transitions of TiCl+ have suggested the presence of perturbations in the ground state, which are also observed in the pure rotational spectrum. The spin–spin constant k derived from the spectroscopic analysis is quite large, indicating a substantial second-order spin–orbit contribution, which likely arises from homogeneous spin-electronic perturbations. The measurement of the spectrum of TiCl+ suggests that other metal ions can be studied using millimeter/submillimeter velocity modulation techniques. [1] N.N. Haese, T. Oka, J. Chem. Phys. 80 (1984) 572–573. [2] B. Lindgren, P. Royen, M. Zackrisson, J. Mol. Spectrosc. 146 (1991) 343–350. [3] S.K. Stephenson, R.J. Saykally, J. Mol. Spectrosc. 231 (2005) 145–153. [4] C.S. Savage, L.M. Ziurys, Rev. Sci. Instrum. 76 (2005) 043106. [5] C.S. Savage, A.J. Apponi, L.M. Ziurys, Astrophys. J. 608 (2004) L73–L76. [6] W.J. Balfour, K.S. Chandrasekhar, J. Mol. Spectrosc. 139 (1990) 245–252. [7] L.A. Kaledin, J.E. McCord, M.C. Heaven, J. Mol. Spectrosc. 173 (1995) 499–509. [8] L.A. Kaledin, M.C. Heaven, J. Mol. Spectrosc. 184 (1997) 113–119. [9] C. Focsa, C. Dufour, B. Pinchemel, I. Hadj Bachir, T.R. Huet, J. Chem. Phys. 106 (1997) 9044–9049. [10] L.A. Kaledin, M.C. Heaven, J. Chem. Phys. 107 (1997) 7020– 7024. [11] C. Focsa, B. Pinchemel, J.-L. Féménias, T.R. Huet, J. Chem. Phys. 107 (1997) 10365–10372. [12] C. Focsa, M. Bencheikh, L.G.M. Pettersson, J. Phys. B-At. Mol. Opt. 31 (1998) 2857–2869. [13] C. Focsa, B. Pinchemel, Chem. Phys. 247 (1999) 395–405. [14] M.A. Flory, D.T. Halfen, L.M. Ziurys, J. Chem. Phys. 121 (2004) 8385–8392. [15] D.T. Halfen, L.M. Ziurys, J. Chem. Phys. 122 (2005) 054309. [16] A. Maeda, T. Hirao, P.F. Bernath, T. Amano, J. Mol. Spectrosc. 210 (2001) 250–258. [17] H. Lefebvre-Brion, R.W. Field, The Spectra and Dynamics of Diatomic Molecules, Elsevier, San Diego, 2004. Acknowledgment This research is supported by NSF Grant CHE0411551.
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