electronic spectroscopy of chbr and cdbr chong tao, calvin mukarakate, mihaela deselnicu and scott...
TRANSCRIPT
Electronic spectroscopy of CHBr and CDBr
Chong Tao, Calvin Mukarakate, Mihaela Deselnicu and Scott A. Reid
Department of Chemistry, Marquette UniversityWisconsin 53233
Simple carbenes
• Carbenes have a divalent carbon
which leads to energetically similar
singlet and triplet states
Typical molecule
S0
T1
S1
Carbene
S0
T1
S1
C C
S0 T1 S1
C
Or reversed
Motivations
• The two lowest singlet states are components of a Renner-Teller pair, and thus simple carbenes are model systems for study of the Renner-Teller effect
• Mapping the singlet-singlet spectra is important for subsequent studies of the triplet state properties
Ene
rgy
X1A
Ã1A
a3A
180o
Methodology
Laser
G
HV
CHBr was produced from pulsed
discharge of CHBr3 precursors
seeded in He, with a backing P=40psi
CDBr was produced from CDBr3
precursor
Spectrum was measured under jet-
cooled condition
Spectra show polyad structure due to similar frequencies of 2 and 3.
Example survey spectra: CHBr
14900 15000 15100 15200 15300
25
1
21
033
0
23
031
0
22
032
0
Inte
nsi
ty
wavenumber in cm-1
24
0
15800 15900 16000 16100
23
033
1
24
032
1
23
032
0
22
033
0
25
0
Inte
nsity
wavenumber in cm-1
24
031
0
At high energies, we also observe levels in the C-H stretching progression.
Example survey spectra: CHBr
18800 19000 19200 19400 19600 198000.00
0.05
0.10
0.15
0.20
0.25
11
024
031
0
11
025
0
11
025
031
0
11
026
0
28
031
0
29
0
Inte
nsi
ty
wavenumber in cm -1
28
0
Br2 dissociation
limit
Example high resolution spectra: CHBr
16940 16950 16960 169700.0
0.2
0.4
0.617830 17840 17850 17860
0.1
0.2
0.3
0.418730 18740 18750 18760
0.0
0.1
Inte
nsi
ty
uncalibrated wavenumber in cm-1
26
0
Inte
nsity 27
0
Inte
nsi
ty 28
0
Dixon plots for CHBr
• Dashed lines are polynomial
fits, solid lines are calculations
of Yu, et al…
• The derived barrier heights
are:
2n 1680 cm-1
2n31 2470 cm-1
2n32 2760 cm-1
15000 16000 17000 18000800
810
820
830
840
850
12000 14000 16000 18000 20000800
820
840
860
880
900
920
14000 16000 18000800
820
840
860
880
900
(G+1 + G/2 in cm -1
2n
032
0
2n
031
0
2n
0
G+
1 - G
(in
cm
-1)
Isotope shifts: CHBr
The isotope shifts with increasing quanta of C-Br stretch (upper panel) are similar for all bands and consistent with a simple harmonic prediction (solid line)
A small dependence of isotope shift on bendingquantum number is observed (lower panel)
0 1 2 3
0
2
4
6
0 2 4 6 81
2
3
4
Isot
ope
shift
[T
(CH
81B
r)-T
(CH
79B
r)]
in c
m-1
m
n = 1n = 2n = 3n = 4n = 5n = 6n = 7n = 8
n
2n
032
0
2n
031
0
2n3m
79Br, 81Br
Excited state C-H stretching frequency
We observe bands in theCH stretching progression(112n) for the first time
A linear extrapolation to n = 0 of the term energy difference between these bands and the 2n bands returns:
E(112n)- E(2n) = 1o +n x12
0
1´ = 3100 cm-1
x120 = -41 cm-1
4 6 82800
2820
2840
2860
2880
2900
Ter
m e
ner
gy
dif
fere
nce
(11 02
n 0-2
n 0)
bending quantum number
Picture of bands observed for CDBr
0 2 4 6 8 10 1213000
14000
15000
16000
17000
18000
19000
20000 2n
2n3
1
2n3
2
112
n
112
n3
1
Waven
um
bers
(cm-1
)
Bending quanta
• Dashed lines are polynomial
fits (third order)
• The derived barrier heights
are:
2n 2110 cm-1
2n31 2890 cm-1
2n32 3501 cm-1
Dixon plots for CDBr
14000 16000 18000
590
600
610
620
630
640
650
660
15000 16000 17000 18000 19000
590
600
610
620
630
640
650
12000 14000 16000 18000
590
600
610
620
630
640
650
660
2n
031
0
[G(v
+1)
-G(v
)] in
cm
-1
[G(v) + G(v+1)]/2 in cm-1
2n
032
0
[G(v
+1)
-G(v
)] in
cm
-1
[G(v
+1)
-G(v
)] in
cm
-1
2n
0
CDBr isotope splitting
1 2 3 4 5 6 7 8 9 10 11 120.40.60.81.01.21.41.61.82.02.22.42.62.83.03.23.4
2n
2n3
1
2n3
2
Iso
top
e s
plit
tin
g in
cm-1
Bending quanta
Excited state C-D stretching frequency
6 8 10
2100
2120
2140
2160
2180
E(1
1 2n )-E
(2n )
Bending quanta
Extrapolated excited stateC-D stretching frequency
1´ = 2351 cm-1
x120 = -25 cm-1
LIF spectra of CHBr/CDBr in the 450-750nm region were recorded and rotationally analyzed.
CH/CD stretching excitation spectra were observed for the first time. Their frequencies were determined to be 3100, and 2351 cm-1, respectively.
The minima in Dixon plots indicate the barrier heights to linearity for CHBr and CDBr are 1680 cm-1
and 2110 cm-1, respectively, above vibrationless level.
Summary
• Members from Dr. Scott Reid’s group
• Funding from NSF and ACS/PRF
Acknowledgements