Rotational Spectroscopy of the Lowest Energy Conformer of 2‑Cyanobutane

Isopropyl
cyanide was recently detected in space as the first branched
alkyl compound. Its abundance with respect to n-propyl
cyanide in the Galactic center source Sagittarius B2­(N2) is about
0.4. Astrochemical model calculations suggest that for the heavier
homologue butyl cyanide the branched isomers dominate over the unbranched n-butyl cyanide and that 2-cyanobutane is the most abundant
isomer. We have studied the rotational spectrum of 2-cyanobutane between
2 and 24 GHz using Fourier transform microwave spectroscopy and between
36 and 402 GHz employing (sub)­millimeter absorption spectroscopy.
Transitions of the lowest energy conformer were identified easily.
Its rotational spectrum is very rich, and the quantum numbers J and Ka reach
values of 111 and 73, respectively. This wealth of data yielded rotational
and centrifugal distortion parameters up to tenth order, diagonal
and one off-diagonal 14N nuclear quadrupole coupling parameters,
and one nuclear spin–rotation coupling parameter. We have also
carried out quantum chemical calculations in part to facilitate the
assignments. The molecule 2-cyanobutane was not found in the present
ALMA data of Sagittarius B2­(N2), but it may be found in the more sensitive
data that have been completed very recently in the ALMA Cycle 4.