Journal of Molecular Structure 695–696 (2004) 385–394
www.elsevier.com/locate/molstruc
Rovibrational analysis of the n4 and n5 þ n9 bands of CHCl2F
Sieghard Albert*, Karen Keppler Albert, Martin Quack*
Laboratorium für Physikalische Chemie, ETH Zürich, Hönggerberg, CH-8093 Zürich, Switzerland
Received 22 December 2003; accepted 22 December 2003
This paper is dedicated to Professor Dr Manfred Winnewisser and Dr Brenda Winnewisser on the occasion of his 70th and her 65th birthday
Abstract
The infrared spectrum of CHCl2F has been measured with a new, very high resolution Fourier transform infrared spectrometer, the Bruker
IFS 120 HR Zürich Prototype (ZP) 2001. The spectrum was recorded with a resolution of 0.0007 cm21 in the range 600– 2300 cm21 at room
temperature. The assignment of the rovibrational transitions has been carried out with the Giessen interactive Loomis – Wood program
developed by Winnewisser et al. [J. Mol. Spectrosc. 136 (1989) 12] and the least squares adjustment has been performed with the Zürich
35
35
21
WANG program. The spectrum has been analyzed in the n4 region of CH Cl2F ðn~0 ¼ 744:474 cm Þ and the n5 þ n9 regions of CH Cl2F
ðn~0 ¼ 829:084 cm21 Þ and CH35Cl37ClF ðn~0 ¼ 825:027 cm21 Þ using an effective Hamiltonian. Both bands are important to understand the
absorption behavior of the fluorochlorohydrocarbon CHCl2F, important in the context of atmospheric pollution as well as in laser chemistry.
Local perturbations have been identified in both bands. The results are discussed in relation to molecular parity violation in the case of the
chiral isotopomer CH35Cl37ClF.
q 2004 Elsevier B.V. All rights reserved.
Keywords: High resolution spectroscopy; Resonance; Infrared; Atmospheric spectroscopy
1. Introduction
The infrared spectra of fluorochlorohydrocarbon molecules and their rovibrational analysis are of crucial
importance for understanding the absorption behavior of
trace gases in the Earth’s atmosphere [2,3] (and references
cited therein) as well as for understanding the infrared laser
chemistry of these compounds [4,5] (and references
therein). It turns out that for many of these compounds
analyses were possible in the past only by using advanced
FTIR and laser spectroscopic techniques in combination
with supersonic jet cooling [6] (and references therein).
Early analyses using these techniques were possible for
CHF2Cl [7,8], CHFCl2 [3] and CFCl3 [9]. However, there
has also been a considerable improvement of resolving
power of commercial FTIR spectrometers over the last two
decades. A first breakthrough arrived with the Bomem
instruments achieving a resolution of about 0.004 cm21
(FWHM, apodized), which led to the early developments in
high resolution FTIR-supersonic jet techniques [10 – 14].
* Corresponding authors. Tel.: þ 41-1-6324421; fax: þ 41-1-6321021.
E-mail addresses: quack@ir.phys.chem.ethz.ch, martin@quack.ch
(M. Quack), albert@ir.phys.chem.ethz.ch (S. Albert).
0022-2860/$ - see front matter q 2004 Elsevier B.V. All rights reserved.
doi:10.1016/j.molstruc.2003.12.047
Another important step was the development of the Bruker
IFS 120 HR instrument with resolutions up to 0.0013 cm21
[15]. The past recent advance was achieved with the Bruker
Zürich prototype 2001 (IFS120 HR ZP 2001), which
achieves an instrumental resolution of about 0.0007 cm21
[16,17]. While the steps in these two later developments
may appear small, at first sight, it turns out that they are very
important because they make possible analyses of the
spectra taken at room temperature for the type of molecules
discussed here, avoiding the need for the complicated jet
cooling experiments. Of course, for even more complex
molecules, cooling techniques in conjunction with the new
spectrometer may become relevant again, not only because
they simplify the spectra recorded, but also because of their
potential in reducing Doppler widths.
We have recorded and analyzed here the FTIR spectrum
of CHCl2F at room temperature in the range of 600–
2300 cm21 [18] at essentially Doppler-limited resolution.
The rovibrational spectra of CH35Cl2F and CH35Cl37ClF
have been already studied by Snels and Quack [3] for the n3 ;
n8 and n7 fundamental bands. However, the resolution of the
analyzed spectra in that work ranged from 0.008 to
0.004 cm21. As a result, the root mean square deviation of
386
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
Table 1
Summary of the fundamentals of CHCl2F (the data for v1 and v2 are from an effective-Resonance Hamiltonian fit [39])
Vibration
Symmetry for C5
isotopomers
n1
n2
n3
n4
n5
n6
n7
n8
n9
a0
a0
a0
a0
a0
a0
a00
a00
a00
CH stretching
CH bending
CF stretching
CCl stretching
CFCl bending
ClCCl bending
CH bending
CCl stretching
CFCl bending
the assigned lines was only drms ¼ 0:0015 – 0:0026 cm21 ;
which was slightly smaller than the error associated with the
determination of line positions from the spectra. The ground
state of CHCl2F has already been analyzed using microwave
[19] and recently, submillimeter wave spectroscopy [20].
Quadrupole coupling constants in the ground state have
been determined [20,21]. Table 1 summarizes the current
knowledge of fundamental vibrations of CHCl2F, including
also the results of the present work.
In this paper, we present the rovibrational analysis of two
further bands of CHCl2F; the n4 fundamental of CH35Cl2F
(CCl stretch, n~0 ¼ 744:47 cm21 ) and the n5 þ n9 combination bands of CH 35Cl 2F ðn~0 ¼ 829:08 cm21 Þ and
CH35Cl37ClF ðn~0 ¼ 825:03 cm21 Þ which are important for
atmospheric absorption [2]. The analysis of an additional
spectral region 900 –2300 cm21 of CHCl2F, in particular of
the 1800 – 2200 cm21 region (the overtone of the CF
stretching mode, 2n3 ) will be presented in separate
publications [22].
The chiral isotopomer CH35Cl37ClF is of potential
importance for general aspects of isotopic chirality and
parity violation [23,24].
2. Experimental
The FTIR spectrum of CHCl2F has been recorded in the
region 600 – 2300 cm 21. The resolution, defined by
1/MOPD (maximum optical path difference) was
0.001 cm21. One hundred and fifty spectra were co-added
in each spectral region.
A White-type cell with a path length ranging from 3.2 up
to 19.2 m was used. The sample pressure was varied from
n~ (cm21)
Reference
CH35Cl2F
CH35Cl37ClF
3024.8
1312
1079.4276
744.474290
458.2
277.2
1239.1940
807.1749
367.4
3024.8
1312
1079.3893
741.4
455.8
274.3
1238.6884
805.0492
365.1
[39]
[39]
[3]
this work, [40]
[40]
[40]
[3],[39]
[3]
[40]
0.09 to 1.3 mbar. An absorption path length of 19.6 m and a
pressure p ¼ 1:3 mbar were used for the n4 band. For the
n5 þ n9 band, the path length was 2.3 m and the pressure
p ¼ 0:5 mbar: Pressure broadening was unimportant under
these conditions.
All spectra were self-apodized. Table 2 shows the
measurement parameters. All spectra were recorded
essentially at Doppler-limitation (Dn~Doppler ¼ 0:0012 cm21
at 1000 cm21 and 295 K). Apertures of 0.8, 1.0 and
1.15 mm were used, which led to instrumental resolutions
of up to 0.0007 cm21. The spectra were calibrated with
OCS [25].
3. Assignment
CHCl2F exists in three isotopomers with a natural
abundance of approximately 9:6:1 (CH 35Cl 2F:
CH35Cl37ClF: CH37Cl2F). Due to the two heavy atoms
and the presence of several isotopomers, the rotational
structure of the bands is dense and congested. Only hybrid
bands have been observed in the spectrum. In this work, the
n4 band of CH35Cl2F and the n5 þ n9 bands of the two major
isotopomers CH35Cl2F and CH35Cl37ClF have been analyzed. In spite of the congested spectrum at room
temperature it was not necessary to decrease the rotational
temperature of the sample in order to simplify the spectra
because the different series of transitions were clearly
visible in the spectra. In the following description, the term
‘subband’ or ‘series’ describes the transitions belonging to
one Ka or Kc value.
The assignment of the observed rovibrational transitions
belonging to a particular subband consisting of P and R
Table 2
Experimental setup for the region 600–1000 cm21 of the infrared spectrum of CHCl2F
Region
(cm21)
Resolution
(cm21)
Windows
Source
Detector
Beamsplitter
Opt. filter
(cm21)
Aperture
(mm)
nmirror
(kHz)
Electr. filter
(cm21)
Calib. gas
600 –1000
0.0007
KBr
Globar
MCT
Ge:KBr
550–1000
0.8, 1.0, 1.15
40
395–1580
OCS [25]
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
branches has been carried out efficiently with an interactive
Loomis –Wood assignment program [1] developed in the
Giessen Laboratory. This method, previously extensively
used for the assignment of linear molecules [26], has been
used successfully for several asymmetric top molecules
(CH35Cl2F, CDBrClF [17] and C2H3DO [27]) because these
molecules display near symmetric top behavior (no
observable asymmetry splitting) at higher J levels.
3.1. The n4 (CCl stretch) band of CH35Cl2F
The n4 band is the weakest band of the nine fundamental
bands of CHCl2F. A sufficient signal-to-noise ratio was only
obtained for the main species CH35Cl2F. a-type transitions
up to J # 91 and c-type transitions up to J # 58 have been
assigned in the spectrum. The a-type series have been
identified as P and R branches with J ^ 1; Ka ; Kc ¼
J ^ 1 2 Ka ˆ J; Ka ; Kc ¼ J 2 Ka : The spacing between
two transitions of a series is approximately 2C: The
assignments have been checked by comparison of the
combination differences (CDs) of the ground state calculated from the assignments of the n3 ; n4 ; n5 þ n9 ; n7 and n8
fundamental bands.
As the Loomis – Wood diagram of the a-type region of
the n4 band of CH35Cl2F in Fig. 1 shows, there are
numerous local resonances. At least three crossings, at
J ¼ 35=39; J ¼ 41=44 and J ¼ 62=67; have been detected.
The perturbations increase with increasing J and Ka
quantum number. The n5 þ n6 and 2n9 levels are the
most likely partners in these interactions with n4.
The c-type subbands shown in Fig. 2 consist also of P
and R branches with J ^ 1; Ka ¼ J ^ 1 2 Kc ; Kc ˆ J;
Ka ¼ J 2 Kc ; Kc : The spacing between two transitions of
387
a series is approximately 2A: Perturbations have not been
detected. As one can see from Figs. 2 and 3, all the ctype R branches are grouped together into three groups.
In contrast, the c-type P branch series are grouped
together into two groups.
It is interesting to note that the c-type transitions have
been assigned only as P and R branch transitions in the n4
and n3 bands. In all the other bands analyzed, n8 ; n7 [18] and
n5 þ n9 ; the c-type transitions have been detected as Q
branch transitions.
3.2. The n5 þ n9 combination band of CH35Cl2F and
CH35Cl37ClF
The signal-to-noise ratio was sufficient to assign the
bands of the two major isotopomers CH35Cl2F and
CH35Cl37ClF. The a-type transitions (J ^ 1; Ka ; Kc ¼
J ^ 1 2 Ka ˆ J; Ka ; Kc ¼ J 2 Ka Þ have been assigned in
P and R branches up to J # 118 for CH35Cl2F, and J # 73
for CH35Cl37ClF whereas the c-type transitions (J; Ka ¼
J 2 Kc ; Kc ˆ J; Ka ¼ J 2 Kc ; Kc ) have been identified as Q
branches up to J ¼ 55 for CH35Cl2F and J ¼ 40 for
CH35Cl37ClF. The Loomis – Wood diagrams in Fig. 4
show a-type transitions of the two major isotopomers
CH35Cl2F (straight series) and CH35Cl37ClF (slanted
series). As can be seen in Fig. 4, the a-type transitions of
CH35Cl2F are locally perturbed at J ¼ 59=67: The 2n6 þ n9
state probably acts as the resonance partner. Within the
observed range of a-type transitions of CH35Cl37ClF, no
crossings have been detected. However, the lines have been
only assigned up to J ¼ 73:
Fig. 1. Loomis–Wood diagram of the a-type transitions of the n4 band of CH35Cl2F in the R branch region. Local perturbations indicated by arrows are visible.
388
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
Fig. 2. Loomis– Wood diagram of the c-type transitions of the n4 band of CH35Cl2F within the R branch region. The transition series are grouped into three
groups. The spectrum in the area of the outlined part of the Loomis–Wood plot between 762.00 and 762.35 cm21 is shown in Fig. 3.
4. Discussion
The rovibrational analysis has been carried out with
Watson’s S and A reduced effective Hamiltonians in the I r
representation up to sextic centrifugal distortion constants
[28] in order to test the different models. The spectroscopic
data have been analyzed with the WANG program described
in detail in Ref. [8].
For the A reduction, the spectroscopic constants of the ground
state constants were fixed to the values of Luis et al. [20] for
CH35Cl2F and CH35Cl37ClF during the fits. For the S reduction,
no ground state values were available. For that reason,
Fig. 3. A comparison of measured R branch transitions (top trace, T ¼ 295 K; path length ¼ 19.6 m, Doppler-limited resolution ¼ 0.0012 cm21) of the n4
band of CH35Cl2F with a simulation (lower trace, resolution ¼ 0.0012 cm21). This is the part of the R branch where the transition series within one group fall
together (see Fig. 2). The noise in the experimental spectrum is visible.
389
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
Fig. 4. Loomis–Wood diagram of the a-type transitions of the n5 þ n9 band of CH35Cl2F. Local perturbations of the different Ka series are visible and indicated
by circles. The slanted series belong to CH35Cl37ClF.
the constants of the ground states of CH35Cl2F and CH35Cl37ClF
have been determined by fitting the CDs calculated from the
assignments of the n3 ; n4 ; n7 ; n8 and n5 þ n8 bands and the
rotational transitions from McLay [19]. The constants are listed in
Table 3 for CH35Cl2F and Table 4 for CH35Cl37ClF.
The deviations of the values of rotational constants of the ground
state fitted by Watson’s S and A reduced Hamiltonians are only
visible in the sixth digit after the decimal point.
For the calculation of the CD, J levels up to J # 90
and Ka # 12 within the a-type transitions of CH35Cl2F
Table 3
Spectroscopic constants in cm21 of the ground state and the n4 and n5 þ n9 states of CH35Cl2F in the S and A reductions
S
n~0
A
B
C
DJ £ 106
DJK £ 106
DK £ 106
d1 £ 106
d2 £ 106
HJ £ 1012
HJK £ 1012
HKJ £ 1012
HK £ 1012
h1 £ 1012
h2 £ 1012
h3 £ 1012
N
drms
Jmax for fit
Jmax assigned
Ka max a-types
Kc max c-types
A
n~0
A
B
C
DJ £ 106
DJK £ 106
DK £ 106
dJ £ 106
dK £ 106
FJ £ 1012
FJK £ 1012
FKJ £ 1012
FK £ 1012
fJ £ 1012
fJK £ 1012
fK £ 1012
n4
Ground state
n5 þ n9
S
A [20]
S
A
S
A
0
0.233 118 37 (91)
0.110 318 6 (37)
0.078 385 11 (65)
0.114 39 (65)
20.118 6 (20)
0.014 7 (14)
20.058 70 (44)
20.027 25 (15)
0.082 4 (78)
–
–
20.092 0 (89)
0.209 (32)
0.150 (29)
0.064 2 (15)
0
0.233 120 688
0.110 316 968
0.078 386 106
0.030 914 1
20.030 286
0.286 28
0.010 091 5
0.057 293 0
0.031 054 8
20.171 11
20.266 85
1.330 92
–
0.306 89
20.540 374
744.474 290 (91)
0.232 929 58 (37)
0.109 705 8 (11)
0.078 102 24 (27)
0.114 63 (89)
20.123 7 (28)
0.018 4 (20)
20.058 38 (48)
20.024 76 (15)
0.082 4
–
–
20.092 0
0.261 (64)
0.150 (66)
0.101 (49)
744.474 354 (71)
0.232 931 66 (17)
0.109 704 30 (58)
0.078 103 09 (23)
0.027 72 (34)
20.009 51 (88)
0.262 9 (10)
20.009 16 (17)
0.062 9 (23)
0.031 054 8
20.171 11
20.266 85
1.330 92
–
0.306 89
20.540 374
829.084 193 (46)
0.232 457 21 (25)
0.110 317 49 (30)
0.078 365 47 (13)
0.112 99 (13)
20.118 10 (37)
0.014 71 (26)
20.055 92 (14)
20.028 444 (74)
20.083 7 (87)
–
–
20.092 0
20.280 (33)
0.558 (30)
0.064 2
829.084 205 (47)
0.232 459 60 (26)
0.110 315 13 (27)
0.078 366 58 (13)
0.033 38 (20)
20.047 13 (90)
0.296 02 (68)
0.011 70 (10)
0.059 72 (70)
20.077 1 (87)
20.171 11
20.266 85
1.150 (61)
–
0.306 89
232.3 (22)
850
0.000 28
90
105
12
27
206
–
80
–
–
–
0.000 34
1230
0.000 34
80
91
7
15
0.000 27
1680
0.000 28
80
118
12
10
If there are no uncertainties listed, the constant was fixed during the fit. The uncertainties given in parentheses one standard deviation in units of the last
digits given.
390
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
Table 4
Spectroscopic constants in cm21 of the ground state and n5 þ n9 state of CH35Cl37ClF in the S and A reductions
A
S
n~0
A
B
C
DJ £ 106
DJK £ 106
DK £ 106
d1 £ 106
d2 £ 106
HJ £ 1012
HJK £ 1012
HKJ £ 1012
HK £ 1012
h1 £ 1012
h2 £ 1012
h3 £ 1012
N
drms
Jmax for fit
Jmax assigned
Ka max a-types
Kc max c-types
n~0
A
A
A
DJ £ 106
DJK £ 106
DK £ 106
dJ £ 106
dK £ 106
FJ £ 1012
FJK £ 1012
FKJ £ 1012
FK £ 1012
fJ £ 1012
fJK £ 1012
fK £ 1012
n5 þ n9
Ground state
S
A [20]
S
A
0
0.231 608 9 (14)
0.107 395 6 (44)
0.076 734 01 (76)
0.119 34 (20)
20.145 7(68)
0.037 0(48)
20.055 5(10)
20.027 9(25)
20.228(57)
–
–
20.295(49)
0.687(12)
0.027 5(64)
0.372(69)
0
0.231 607 360
0.107 392 039
0.076 735 753
0.029 401
0.029 350
0.283 840
0.009 538 1
0.055 748 6
0.031 215
20.160 778
20.286 532
1.330 92
–
0.306 89
20.540 374
825.027 526 (51)
0.230 951 60 (62)
0.107 385 47 (33)
0.076 699 149 (93)
0.111 50 (48)
20.133 07(61)
0.031 92(21)
20.053 08(30)
20.031 57(16)
20.235 3(61)
–
–
20.295
0.569(27)
0.027 5
0.372
825.027 505 (35)
0.230 950 68 (56)
0.107 382 30 (17)
0.076 700 761 (37)
0.031 029 (86)
20.005 09(75)
0.312 3(13)
0.010 509(43)
0.049 40(42)
0.031 215
20.160 778
20.286 532
1.330 92
–
0.306 89
20.540 374
580
0.000 31
67
83
8
17
125
–
60
–
–
–
1080
0.000 28
0.000 28
66
73
9
10
If there are no uncertainties listed, the constant was fixed during the fit. (See also table 3).
and J # 65 and Kc # 27 within the c-type transitions of
CH35Cl2F were used. For CH35Cl37ClF, J # 65 and
Ka # 8 within the a-type transitions and J # 55 and
Kc # 17 within the c-type transitions were used. The
sextic constants HJK and HKJ of Watson’s S reduced
Hamiltonian could not be determined and were set to
zero for CH35Cl2F and CH35Cl37ClF. In total 850 CD of
CH35Cl2F and 580 CD of CH35Cl37ClF were used. The
standard deviation is slightly better for the CH35Cl2F
isotopomer than for the CH35Cl37ClF isotopomer because
the signal-to-noise ratio of the CH35Cl2F absorption lines
is higher.
Based on these fixed ground state constants, the constants
of the n4 level of CH35Cl2F and the n5 þ n9 levels of
CH35Cl2F and CH35Cl37ClF were determined. These are
shown in Tables 3 and 4. Local resonances of the involved
bands have been neglected during the fit by not including
transitions in perturbed regions. The sextic constants HJK
and HKJ of Watson’s S reduced Hamiltonian of the n4 level
were set to zero as was also done for the ground state. In
addition, HJ and HK were fixed to the values of the ground
state. The sextic constants could not be determined for the A
reduced Hamiltonian of the n4 level and were fixed to the
values of the ground state. The standard deviations drms for
the fits of the n4 level are identical for both models (S and A
reduced Hamiltonians).
The spectrum of the n4 band for CH35Cl2F was simulated
based on these constants and was identical for both
reductions. A comparison of the measured and simulated
c-type R branch lines is shown in Fig. 3. This is the part of
the R branch region in which the series within the three
groups fall together. The same part of the spectrum
(762.00 – 762.35 cm21) is outlined in the Loomis – Wood
diagram in Fig. 2. The agreement between simulation and
experiment in Fig. 3 is quite good. It is evident that there are
more lines in the measured spectrum than in the simulation.
These extra lines belong probably to the CH35Cl37ClF
isotopomer. However, the relatively high noise level of the
recorded spectrum is clearly visible. This makes it
practically impossible to recognize series of absorption
lines of the CH35Cl37ClF isotopomer in this region. A
comparison of the change of the rotational constant B upon
excitation of the modes n3 ; n4 ; n7 ; n8 and n5 þ n9 [3,18]
shows the largest change upon excitation of n4 (Table 3).
The sextic constants HJK and HKJ of the S reduction for
the n5 þ n9 levels of CH35Cl2F and CH35Cl37ClF could also
not be determined and were set to zero. In addition, the HK
and h3 constants for CH35Cl2F and HK and h2 and h3 for
CH35Cl37ClF were fixed to the values for the ground state.
As the standard deviations show for the two isotopomers,
the anharmonic resonance mentioned in the paper of Snels
and Quack [3] can be neglected for a line-by-line assignment of individual bands, providing effective parameters
only. However, the large value of fK of CH35Cl2F for the A
reduction is an indicator of a hidden global resonance. For
CH 35Cl 2F the sextic constants FJ ; FK and fK of
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
391
Fig. 5. A comparison of the measured Q branches (c-type transitions) of the n5 þ n9 band of CH35Cl2F (top trace, T ¼ 295 K; path length ¼ 19.6 m,
p ¼ 0:5 mbar; Doppler-limited resolution ¼ 0.0012 cm21) with a simulation of CH35Cl2F and CH35Cl37ClF (lower trace, resolution ¼ 0.0012 cm21).
‘the A reduction have been determined. For CH35Cl37ClF,
no sextic constants in the A reduction could be determined.
All the constants were fixed to the values of the ground state.
The standard deviations drms for the both reduced Hamiltonians are again identical for both isotopomers.
The simulation of the n5 þ n9 band based on the fitted
constants, again identical for both models, illustrates an
excellent agreement with the measured spectrum. Fig. 5
shows a comparison of measured and simulated c-type Q
branch lines of CH35Cl2F up to J ¼ 54: A part of the Q
branch is enlarged in Fig. 6 to demonstrate the resolution of
the new Zurich spectrometer. Even for the weaker lines, atype R branch lines of CH35Cl37ClF and a-type P branch
lines of CH35Cl2F at low J values, the agreement between
Fig. 6. A comparison of an expanded part of the measured Q branch lines of the n5 þ n9 band of CH35Cl2F (top trace, T ¼ 295 K; path length ¼ 19.6 m,
p ¼ 0:5 mbar; Doppler-limited resolution ¼ 0.0012 cm21) with a simulation of CH35Cl2F and CH35Cl37ClF (lower trace, resolution ¼ 0.0012 cm21). Parts of
the a-type P branches of CH35Cl2F and R branches of CH35Cl37ClF are also visible.
392
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
Fig. 7. A comparison of the measured Q branches of CH35Cl37ClF and P branches of CH35Cl2F of the n5 þ n9 band (top trace, T ¼ 295 K; path
length ¼ 19.6 m, p ¼ 0:09 mbar; Doppler-limited resolution ¼ 0.0012 cm21) with a simulation of CH35Cl37ClF and CH35Cl2F (lower trace,
resolution ¼ 0.0012 cm21).
recorded and simulated spectrum is superb. Another
example is shown in Fig. 7. Due to the high resolving
power of the spectrometer we can partially resolve Q branch
features. In addition to c-type transitions of Q branches of
CH35Cl37ClF there are strong a-type P branches of
CH35Cl2F. A part of the a-type P branches of CH35Cl2F is
shown in Fig. 8. In spite of a fairly high noise level, the
agreement between measurement and simulation is very
Fig. 8. A comparison of a part of the measured P branches of the n5 þ n9 band of CH35Cl2F (top trace, T ¼ 295 K; p ¼ 1:3 mbar; path length ¼ 19.6 m,
Doppler-limited resolution ¼ 0.0012 cm21) with a simulation of CH35Cl2F and CH35Cl37ClF (lower trace, resolution ¼ 0.0012 cm21).
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
good. The patterns of the a-type transitions are clearly
visible.
5. Conclusions
The recording and assignment of congested and
complicated spectra of relatively heavy molecules ðm $
100 DaÞ is much simpler with the higher resolution
available with our new spectrometer because we can
avoid complicated supersonic jet cooling techniques. The
spectra can be recorded at room temperature, which saves
a great deal of time and effort. The Giessen Loomis –
Wood assignment program [1] is very helpful in assigning
the spectra of prolate and oblate asymmetric rotors and
the WANG program [8] provides a fairly universal tool in
fitting effective Hamiltonian constants to complex band
systems. Watson’s reduced A and S Hamiltonians both
reproduce the recorded spectra very well for the bands
analyzed here.
We have analyzed for the first time the rovibrational
structure of the n4 band of CH35Cl2F and the combination
band n5 þ n9 of CH35Cl2F and CH35Cl37ClF. Both bands are
of importance for a complete understanding of the
absorption behavior of the fluorochlorohydrocarbon
CHCl2F in the Earth’s atmosphere. Due to the high
resolving power of our spectrometer, we are now able to
detect local resonances which could not be observed in
earlier studies [3]. The assignment of the bands showed that
the a-type transitions of the n4 and n5 þ n9 bands of
CH35Cl2F are locally perturbed. Interesting resonances were
found in the previously assigned bands n3 and n7 of
CH35Cl2F. In particular, the n3 band illustrates perturbations
in the a- and c-type transitions. The analysis of these bands
and the 2n3 band will be the subject of a future paper [22].
Bands of the chiral isotopomer CH35Cl37ClF which
fall within the CO2 laser region are of interest for laser
chemistry [4,5] and for a future detection of molecular
parity violation. The present analysis makes it possible to
identify unperturbed regions in the spectrum of
CH35Cl37ClF in which CO2 laser spectroscopy can be
conducted. In particular, the 2n3 band is of interest
because quasiresonantly enhanced two photon CO2 laser
transitions can be used for this band. With the previous
ground work on isotopic chirality in general, presented in
Refs. [23,24,29] and here for the isotopomer
CH35Cl37ClF, in particular, it might be possible to detect
rovibrational absorption line shifts due to parity violation
[30,31]. Another possibility to detect rotational line shifts
is presented by submillimeter wave spectroscopy. Backward wave oscillators [32,33] have spectral purities
smaller than 1 Hz. If they are phase locked they reach
a resolving power of Dn=n ¼ 3 £ 10213 [32]. This ratio is
probably not good enough for the chiral isotopomer
CH35Cl37ClF, but it may be sufficient for heavier
molecules [23,24,34,35].
393
Another more obvious application of the present results
concerns atmospheric spectroscopy. The importance of
detailed rovibrational analyses for a correct interpretation of
remote sensing experiments as well as for quantitative
detection of tropospheric freons has been emphasized
repeatedly [36– 38]. In the aftermath of the Montreal
protocol banning the fluorochlorocarbons, the fluorochlorohydrocarbons may become more important in the future.
These are considered less problematic because of their
shorter lifetimes, which are due to kinetic decay by
chemical attack at the H-atom. In this context, we are also
working on a new determination of the absolute band
strengths of the most important bands [22].
Acknowledgements
Our work is financially supported by the Schweizerische
Nationalfonds and the ETH Zürich (including AGS, CSCS
and C4). We enjoyed discussions with Michael Hippler,
Hans Hollenstein, Achim Sieben, Jürgen Stohner, Andreas
Steinlin and Martin Willeke.
References
[1] B.P. Winnewisser, J. Reinstädtler, K.M.T. Yamada, J. Behrend,
J. Mol. Spectrosc. 136 (1989) 12–18.
[2] C.P. Rinsland, D.W. Johnson, A. Goldman, J.S. Levine, Nature 337
(1985) 535.
[3] M. Snels, M. Quack, J. Chem. Phys. 95 (1991) 6355–6361.
[4] D.W. Lupo, M. Quack, Chem. Rev. 87 (1987) 181–216.
[5] M. Quack, Infrared Phys. 29 (1989) 441– 466.
[6] M. Quack, Annu. Rev. Phys. Chem. 41 (1990) 839– 874.
[7] A.J. Ross, A. Amrein, D. Luckhaus, M. Quack, Mol. Phys. 66 (1989)
1273– 1277.
[8] D. Luckhaus, M. Quack, Mol. Phys. 68 (1989) 745 –758.
[9] M. Snels, A. Beil, H. Hollenstein, M. Quack, U. Schmitt, F. D’Amato,
J. Chem. Phys. 103 (1995) 8846–8853.
[10] H.-R. Dübal, M. Quack, U. Schmitt, Chimia 38 (1984) 438– 439.
[11] A. Amrein, M. Quack, U. Schmitt, Mol. Phys. 60 (1987) 237–248.
[12] A. Amrein, M. Quack, U. Schmitt, Z. Phys. Chem. N.F. 154 (1987)
59–72.
[13] A. Amrein, M. Quack, U. Schmitt, J. Phys. Chem. 92 (1988)
5455– 5466.
[14] A. Amrein, D. Luckhaus, F. Merkt, M. Quack, Chem. Phys. Lett. 152
(1988) 275–280.
[15] M. Birk, M. Winnewisser, E.A. Cohen, J. Mol. Spectrosc. 136 (1989)
420–443.
[16] S. Albert, M. Quack, Chimia 56 (2002) 374.
[17] S. Albert, K.K. Albert, M. Quack, FTS OSA Tech. Digest (2003) 177.
[18] S. Albert, M. Quack, In Eighteenth Colloquium on High Resolution
Molecular Spectroscopy, Paper D37, 2003, p. 145 Dijou France.
[19] D.B. McLay, Can. J. Phys. 42 (1964) 720.
[20] A. Luis, J.C. Lopez, A. Guarnieri, J.L. Alonso, J. Mol. Struct. 413
(1997) 249–253.
[21] J.C. Lopez, A. Luis, S. Blanco, A. Lesarri, J.L. Alonso, J. Mol. Struct.
612 (2002) 287 –303.
[22] S. Albert, M. Quack, A. Steinlin, in preparation.
[23] M. Quack, Angew. Chem. Int. Ed. (Engl.) 28 (1989) 571–586.
[24] M. Quack, Angew. Chem. Int. Ed. (Engl.) 114 (2002) 4812–4825.
394
S. Albert et al. / Journal of Molecular Structure 695 –696 (2004) 385–394
[25] A.G. Maki, S. Wells, Wavenumber calibration tables from
heterodyne frequency measurements, NIST Special Publication
821, USA, 1991.
[26] S. Albert, M. Winnewisser, B.P. Winnewissser, Ber. Bunsenges. Phys.
Chem. 100 (1996) 1876–1896.
[27] K.K. Albert, S. Albert, M. Quack, J. Stohner, O. Trapp, V. Schurig, In
Eighteenth Colloquium on High Resolution Molecular Spectroscopy,
Paper F38, 2003, p. 202 Dijou, France.
[28] J.K.G. Watson, in: J.R. Durig (Ed.), Vibrational Spectra and Structure,
vol. 6, Elsevier, Amsterdam, 1978, pp. 1–89.
[29] R. Berger, M. Quack, A. Sieben, M. Willeke, in preparation.
[30] M. Quack, J. Stohner, Phys. Rev. Lett. 84 (2000) 3807–3810.
[31] M. Quack, J. Stohner, J. Chem. Phys. 119 (2003) 11228–11240.
[32] F. Lewen, R. Gendriesch, I. Pak, D. Paveliev, R. Hepp, M. Schieder,
G. Winnewisser, Rev. Sci. Instrum. 69 (1998) 32.
[33] D.T. Petkie, T.M. Goyette, R.P.A. Bettens, S.P. Belov, S. Albert, P.
Helminger, F.C. De Lucia, Rev. Sci. Instrum. 68 (1997) 1675– 1683.
[34] R. Schwerdtfeger, J. Gierlich, T. Bollwein, Angew. Chem. Int. Ed. 42
(2003) 1293–1296.
[35] M. Gottselig, M. Quack, J. Stohner, M. Willeke, Int. J. Mass.
Spectrum (2004) in press.
[36] N. Van-Thank, I. Rossi, A. Jean-Louis, H. Rippel, J. Geophys. Res.
D. Atmos. 91 (1986) 4056–4062.
[37] D.P. Kratz, P. Varanasi, J. Quant. Spectrosc. Radiat. Transfer 48
(1992) 245 –254.
[38] S.T. Massie, P. Goldman, J. Quant. Spectrosc. Radiat. Transfer 48
(1992) 713 –719.
[39] H.-R. Dübal, M. Quack, Mol. Phys. 53 (1984) 257–264.
[40] A. Baldacci, A. Passerini, S. Ghersetti, Spectrochim. Acta, Part A 40
(1984) 165 –171.