C2H5OH
Ethanol, v = 0
Species tag 046524
Version1*
Date of EntryNov. 2016
ContributorH. S. P. Müller

Ethanol, aka ethyl alcohol, occurs in two distinguishable conformers because of the orientation of the OH group. The internal rotation of the CH3 group can be neglected in most instances. The anti conformer is lowest in energy, the doubly degenerate gauche conformer is about 58 K higher in energy. Tunneling between the two equivalent gauche conformers lifts the degeneracy, causing a gauche+ and a gauche state which interact heavily.
The present entry is a modification of the JPL catalog entry which is based on
(1) J. C. Pearson, C. S. Brauer, B. J. Drouin, 2008, J. Mol. Spectrosc. 251, 394.
The modifications were described by
(2) H. S. P. Müller, A. Belloche, L.-H. Xu, R. M. Lees, R. T. Garrod, A. Walters, J. van Wijngaarden, F. Lewen, S. Schlemmer, and K. M. Menten, 2016, Astron. Astrophys. 587, Art. No. A92.
Basically, it is a recalculation of the data provided in the JPL catalog archive with a change in one of the signs of the dipole moment components. The recalculation together with the modified sign resolves intensity problems pointed out already in (1) and that were also noticed in (2).
Extensive sets of transition frequencies were determined in (1) along with very accurate energies of the gauche substates. Additional data for the anti conformer originate from
(3) J. C. Pearson, K. V. L. N. Sastry, M. Winnewisser, E. Herbst, F. C. De Lucia, 1995, J. Phys. Chem. Ref. Data 24, 1;
and from references therein. Additional data for the gauche conformer originate from
(4) J. C. Pearson, K. V. L. N. Sastry, E. Herbst, F. C. De Lucia, 1996, J. Mol. Spectrosc. 175, 246;
from
(5) J. C. Pearson, K. V. L. N. Sastry, E. Herbst, F. C. De Lucia, 1996, Astrophys. J. 480, 420;
and from references therein.
Predictions may be good as long as the predicted uncertainties do not exceeed 200 or 300 kHz. We refrained from merging experimental lines; we recommend to inspect the fit file for experimental lines, their uncertainties, and their residuals.
Note: The partition function takes into account the ground vibrational states only. Approximate vibrational correction factors should be available soon.
The dipole moment components of the anti conformer were determined by
(1) M. Takano, Y. Sasada, and T. Satoh, 1968, J. Mol. Spectrosc. 26, 157
those of the gauche conformer by
(7) R. K. Kakar and C. R. Quade, 1980, J. Chem. Phys. 72, 4300.
Note: State number 2 signals the lowest energy anti conformer, state numbers 0 and 1 the symmetric and antisymmetric gauche conformer substates.

Lines Listed69527
Frequency / GHz< 1000
Max. J86
log STR0-8.5
log STR1-7.5
Isotope Corr.-0.0
Egy / (cm–1)0.0 / 39.54, 42.77
 µa / D0.05 / 1.26
 µb / D1.44 / 0.10
 µc / D0.00 / 1.10
 A / MHz34921. / 34186.
 B / MHz9351.2 / 9191.8
 C / MHz8138.5 / 8097.3
 Q(300.0)45601.2912
 Q(250.0)33853.1288
 Q(225.0)28439.8942
 Q(180.0)19556.0038
 Q(150.0)14312.3251
 Q(120.0)9684.0548
 Q(75.00)4106.4006
 Q(37.50)1072.4178
 Q(18.75)290.9463
 Q(9.375)95.5970
 Q(5.000)37.5425
 Q(2.725)15.4354
detected in ISM/CSMyes


Database maintained by Holger S. P. Müller and Sven Thorwirth, programming by D. Roth and F. Schlöder