Open AccessHyperfine excitation of HCN by H 2 at low temperature
Author(s) -
Ben Abdallah D.,
Najar F.,
Jaidane N.,
Dumouchel F.,
Lique F.
Publication year - 2012
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1111/j.1365-2966.2011.19896.x
Subject(s) - hyperfine structure , atomic physics , physics , collisional excitation , excitation , rotational transition , rotational temperature , excited state , spectral line , ab initio , hydrogen , angular momentum , ionization , ion , astronomy , quantum mechanics
Modelling of molecular emission spectra from interstellar clouds requires the calculation of rate coefficients for (de‐)excitation by collisions with the most abundant species. We calculate rate coefficients for the rotational and hyperfine (de‐)excitation of the hydrogen cyanide (HCN) by collisions with H 2 ( j = 0), the most abundant collisional partner in cold molecular clouds. The scattering calculations are based on a new ab initio potential energy surface for the HCN–H 2 collisional system, averaged over the H 2 orientations. Close‐coupling calculations of pure rotational cross‐sections are performed for levels up to j = 10 and for total energies up to 1000 cm −1 . The hyperfine cross‐sections are then obtained using a recoupling technique. The rotational and hyperfine cross‐sections are used to determine collisional rate coefficients for temperatures ranging from 5 to 100 K. A clear propensity rule in favour of even Δ j rotational transitions is observed. The usual Δ j =Δ F propensity rules are observed for the hyperfine transitions. The new rate coefficients are compared with the previous results obtained for the HCN molecule. Significant differences are found, mainly due to the use of H 2 as a collisional partner instead of He. The new rate coefficients will significantly help in interpreting HCN emission lines observed with current and future telescopes.