The exploration of phosphorus-bearing species stands
as a prolific
field in current astrochemical research, particularly within the context
of prebiotic chemistry. Herein, we have employed high-level quantum
chemistry methodologies to predict the structure and spectroscopic
properties of isomers composed of a methyl group and three P, C, and
O atoms. We have computed relative and dissociation energies, as well
as rotational, rovibrational, and torsional parameters using the B2PLYPD3
functional and the explicitly correlated coupled cluster CCSD(T)-F12b
method. Based upon our study, all the isomers exhibit a bent heavy
atom skeleton with CH3PCO being the most stable structure,
regardless of the level theory employed. Following in energy, we found
four high-energy isomers, namely, CH3OCP, CH3CPO, CH3COP, and CH3OPC. The computed adiabatic
dissociation energies support the stability of all [CH3, P, C, O] isomers against fragmentation into CH3 and
[P, C, O]. Torsional barrier heights associated with the methyl internal
rotation for each structure have been computed to evaluate the occurrence
of possible A–E splittings
in the rotational spectra. For the most stable isomer, CH3PCO, we found a V
3 barrier of 82 cm–1, which is slightly larger than that obtained experimentally
for the N-counterpart, CH3NCO, yet still very low. Therefore,
the analysis of its rotational spectrum can be anticipated as a challenging
task owing to the effect of the CH3 internal rotation.
The complete set of spectroscopic constants and transition frequencies
reported here for the most stable isomer, CH3PCO, is intended
to facilitate eventual laboratory searches.