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THE MICROWAVE SPECTRA OF THE LINEAR OC HCCCN,
OC DCCCN, AND THE T-SHAPED HCCCN CO2 COMPLEXES
The 62nd. International Symposium on Molecular Spectroscopy, RG 09
LU KANGDepartment of Natural Sciences, Union College, Barbourville, KY 40906
STEWART E. NOVICKDepartment of Chemistry, Wesleyan University, Middletown, CT 06459
General Introduction
IR study of the OC---HCCCN, and the HCCCN---CO2
X. Yang, R.Z. Pearson, G. Scoles; Chem. Phys. Lett., 204(12), p145, 1993X. Yang, R.Z. Pearson, and G. Scoles; J. Mol. Spectrosc., 180(1), p1, 1996
Rotational spectroscopy study of the OC---HCNE. J. Goodwin, A. C. Legon; Chem. Phys., 87, p81, 1984
Both Linear and T-shaped HCN---CO2 exist
T. D. Klots, R. S. Ruoff, H. S. Gutowsky; J. Chem. Phys., 90(8), p4216, 1989K. R. Leopold, G. T. Fraser, W. Klemperer; J. Chem. Phys., 80(3), p1039, 1984
Complete rotational spectroscopy investigations of the weakly bound Ng---HCCCN van der Waals complexes He---HCCCN: W. C. Topic, W. Yäger; J. Chem. Phys.,123(6), p064303/1, 2005 Ne---HCCCN: A. Huckauf, W. Yäger; manuscript in preparation. Ar---HCCCN: A. Huckauf, W. Yäger, P. Botschwina, R. Oswald; J. Chem. Phys., 119(15), p7749, 2003
Thorough understanding of the subunits: CO and HCCCNCO: F. J. Lovas, P. H. Krupenie; J. Phys. Chem. Ref. Data, 3(1), p245, 1974HCCCN: W. J. Lafferty, F. J. Lovas; J. Phys. Chem. Ref. Data, 7(2), p441, 1978
Experiment
Balle-Flygare Type Fourier transform microwave spectrometer (FTMW) at Wesleyan University Molecular beam pulsed-nozzle (~3 K) Cover 3.7 – 26.5 GHz ~ 1 kHz frequency resolution
The synthesis of Ethyl cyanide (Cyanoacetylene), HCCCN. C. Moureu, J. C. Bongrand; Ann. Chim. (Paris), 14, p47, 1920. Propiolamide is commercially available (Acme Bioscience Inc.)
Deuterated sample, DCCCN was also made! 0.5% HCCCN (DCCCN) + 7.5% CO / Ar or Ne carrier gas 0.5% HCCCN (DCCCN) + 10% CO2 / Ar or Ne carrier gas
H C C C
O
NH2
H C C C N120 - 140 oC
+ P2O5sand
Hamiltonian
H = HR + HQ
HR: the effective Hamiltonian for the vibrational ground state semi-rigid linear molecules
HR = B0J2 – D0J4 + H0J6
EJ = B0J(J+1) – D0J2(J+1)2 + H0J3(J+1)3
J+1→J = 2B0(J+1) – 4D0(J+1)3 + H0(J+1)3[(J+2)3-J3]
HQ: the nuclear quadrupole coupling interactions between the molecular rotation angular momentum, J, and the nuclear spin angular momentum, I.
HQ = The nuclear spin of Nitrogen atom is1, hence, J + I(N) = F
EQ :6
1
Spectroscopic constants
Table-1: the rotational constants, centrifugal distortion constants, and the nuclear quadrupole coupling constants of the OC---HCCCN isotopomers Molecular Species
(Hydrogenated) B0
(MHz) D0
(kHz) H0
(Hz) eqQ(14N) (MHz)
σ (kHz) / # of lines
18OC --- HCCCN 591.143890(36) 0.29866(29) -0.386(67) -4.2097(19) 1.4 / 32
O13C --- HCCCN 611.097110(30) 0.31732(21) -1.52(49) -4.2085(10) 1.0 / 44
OC --- HCCCN 619.521775(21) 0.32577(11) -0.39(18) -4.20865(55) 0.74 / 72
OC --- H13CCCN 619.376060(39) 0.32520(28) -0.47(55) -4.2123(19) 1.0 / 32
OC --- HC13CCN 617.799558(32) 0.32443(23) -1.10(47) -4.2085(15) 1.0 / 37
OC --- HCC13CN 613.348720(32) 0.31871(23) -0.05(47) -4.2096(20) 0.72 / 38
OC --- HCCC15N 607.553100(56) 0.30901(23) -0.70(68) N/A 0.85 / 14
Spectroscopic constants
Table-1: the rotational constants, centrifugal distortion constants, and the nuclear quadrupole coupling constants of the OC---DCCCN isotopomers
Molecular Species (Deuterated)
B0 (MHz)
D0 (kHz)
H0 (Hz)
eqQ(14N) (MHz)
# of lines / σ (kHz)
18OC --- DCCCN 591.397792(45) 0.28887(37) 2.76(92) -4.354(65) 3.0 / 28
O13C --- DCCCN 611.289802(30) 0.30730(29) -0.02(65) -3.928(35) 1.9 / 36
OC --- DCCCN 619.654917(32) 0.31430(25) -0.58(58) -4.21113(66) 1.8 / 57
OC --- D13CCCN N/A N/A N/A N/A N/A
OC --- DC13CCN 617.915477(39) 0.31292(29) -1.85(66) -4.244(35) 1.7 / 33
OC --- DCC13CN 613.442390(39) 0.30814(30) 1.45(67) -4.125(35) 2.3 / 35
OC --- DCCC15N 607.631979(78) 0.30238(72) 0.0102(20) N/A 3.5 / 11
Spectroscopic constants of HCCCN---CO2
Table-3: The spectroscopic constants of the T-shaped HCCCN---CO2 dimer
Constants * A / MHz 11824 B / MHz 764.597(3) C / MHz 715.745(2) ΔJ / kHz 0.5006(7)
ΔJK / kHz 120.89(4) δJ / kHz 0.0425(11) δK / kHz 0.0653(6) HJ / kHz 1.2(11) 10-6
HJK / kHz 0.03488(9) HKJ / kHz -0.683(3) HK / kHz 2.52779(5) χaa / MHz -4.1293(3)
χbb – χcc / MHz 0.10(8) σ / kHz 1.5
# of lines 214 *: The standard deviations are put in the ( ). : Fixed to HCN---CO2 value, 0.394406 cm-1.
The observed spectra agree with the T-shaped structure.
IR spectroscopy determined rotational constants:
B” = 0.0254463(59) cm-1
i.e., 762.9(19) MHz
C” = 0.0254463(59) cm-1
i.e., 715.5(18) MHz
X. Yang, R. Z. Pearson, G. Scoles;
J. mol. Spectro.180, p 1-6, 1996 The obtained rotational constants
from the microwave spectroscopy are in good agreement with the IR values.
Structural Analysis: Linear Model
a C O C C C H N
a
r c .m .
r c - c
rO C - - - H C
b
b
IR spectroscopy determined rOC-HC = 2.615Å for OC---HCCCN complex Yang, et. al., Chem. Phys. Lett., 204(12), p145-151, 1993. Microwave spectroscopy determined rOC-HC = 2.577Å for OC---HCN Goodwin, et. al., Chem. Phys., 87, p81-92, 1984.
Structural Analysis: Linear Model
How to find a distance that can best descrbe the complex?Table-4: Various distances related to the linear model of OC---HCCCN and OC---DCCCN*
Molecular Species rc.m. (Å) rc-c (Å) rOC-HC (Å)
OC---HCCCN 6.2048 3.6610 2.6035 18OC---HCCCN 6.2361 3.6600 2.6024
O13C---HCCCN 6.1827 3.6613 2.6038
OC---H13CCCN 6.1687 3.6615 2.6040
OC---HC13CCN 6.1916 3.6611 2.6036
OC---HCC13CN 6.2179 3.6608 2.6034
OC---HCCC15N 6.2401 3.6609 2.6034
OC---DCCCN 6.1443 3.6575 2.6005 18OC---DCCCN 6.1756 3.6564 2.5994
O13C---DCCCN 6.1222 3.6578 2.6007
OC---D13CCCN N/A N/A N/A
OC---DC13CCN 6.1324 3.6576 2.6006
OC---DCC13CN 6.1588 3.6579 2.6008
OC---DCCC15N 6.1800 3.6574 2.6004
*Kisiel’s STRFIT program gives us rOC-HC = 2.6018(5) Å
Structural Analysis: Procession Model
The description of the procession model: E. J. Goodwin & A. C. Legon; Chem. Phys., 87, p81 – 92, 1984
C
N
C
C
H
C
O
a a
b
b rc.m.
rOC--HC
rc-c
θ
HCCCNCO
HCCCNCO
HCCCNb
CObmcbb
MM
MM
IIrI
222.. cos1
2
1cos1
2
1
Structural Analysis: Procession Model
Average effect of the procession around the a-axis
The geometry of the complex is determined by rc.m. and θ, , µ,
can be obtained from the experiment.
can be obtained from the quadrupole coupling constant of 14N
222..
exp cos12
1cos1
2
1 HCCCN
bCObmcbbb IIrII
expb
HCCCNb
COb I,I,I
1cos32
1 20 aa
1
)(
)(2
3
1cos
140
142
N
Naa
1
)(
)(2
3
1arccos
140
14
N
Naa
02
020
21
2
2
ddd aaaaaa
Structural Analysis: Procession Model
For example, OC---HCCCN, aa(14N)=-4.20865(55)MHz, and the 0(14N) for free HCCCN is: 0(14N)=-4.31806(38)MHz, then: OC---HCCCN: =7.468(1)
For other isotopomers: OC---DCCCN: =7.31(4)18OC---HCCCN: =7.432(3) 18OC---DCCCN: N/AO13C---HCCCN: =7.473(1) O13C---DCCCN: =14.17(2)OC---H13CCCN: =7.341(3) OC---D13CCCN: N/AOC---HC13CCN: =7.473(1) OC---DC13CCN: =6.05(6)OC---HCC13CN: =7.435(1) OC---DCC13CN: =9.89(3)OC---HCCC15N: N/A OC---DCCC15N: N/A
= 7.44(5) ↔ OC---HCN = 13-14
Structural Analysis: Procession Model
Ibb is determined by the (θ, r2c.m.½) pair, how do we estimate θ?
Note that rc-c is almost isotropically invariant, and, (θ, rc-c) can also be used to determine Ibb, i.e., Ib
exp
Construct a set of (θ, rc-c) pairs from the main isotopomer and use them to reproduce Ibbs for other isotopomers, and find the best matched (θ, rc-c) pair to get the answer.
Examples: 18OC---HCCCN: O13C---HCCCN:
comparing with 18OC---HCN: ~ 15º O13C---HCN: ~ 10º
The procession model does not work very well for HCCCN isotopomers! ~ 0º - 90º (similar to the OC---HCN when use this model to handle HCN isotopomers!)
MHz144.591Bexp0 MHz140.591B 16
0
MHz097.611Bexp0 MHz100.611B 8
0
Conclusion
1. The rotational spectra of the weakly bound van der Waals complex dimers, including, OC---HCCCN, OC---DCCCN, and HCCCN---CO2 are observed.
2. All 13C (1.07%), 15N (0.37%), and 18O (0.205%) isotopomers are found in natural abundance!
3. The obtained results are in good agreement with previous studies
4. OC---HCCCN / OC---DCCCN is linear shaped. The procession model is effective to describe this system.
5. The T-shaped HCCCN---CO2 has been observed. We tried, but the linear shaped CO2---HCCCN was not found yet!
6. Why the procession model failed to reproduce the geometry of the OC---HCCCN complex when the HCCCN subunit is substituted by 13C or 15N isotopes?
Future Plan
1. Try to improve the quality of the data for OC---DCCCN by observing low frequency transitions. (get the eqQ for D).
2. Try to get the nuclear quadrupole coupling splittings due to the 13C of O13C-HCCCN. (can help us figure out very accurately)
3. Keep searching for the linear shaped CO2---HCCCN dimer.
4. We already observed N2---HCCCN.
5. We already observed HCCCN---HCCCN, HCCCN---DCCCN, DCCCN---HCCCN, and DCCCN---DCCCN dimers (The low frequency data will really help!).
6. Searching for NO---HCCCN complex.