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Table · dataset · 2024

Rovibrational (de-)excitation of H2 by He

Listed in IVOA Registry (Virtual Observatory)

The collisional (de-)excitation of H_2_ by He plays an important role in the thermal balance and chemistry of various astrophysical environments, making accurate rate coefficients essential for interpreting observations of the interstellar medium.

Description

Our goal is to utilize a state-of-the-art potential energy surface (PES) to provide comprehensive state-to-state rate coefficients for He-induced transitions among rovibrational levels of H_2_.

We performed quantum scattering calculations for the H_2_-He system. Thus, we were able to provide state-to-state rate coefficients for 1059 transitions between rovibrational levels of H_2_, with internal energies up to 15000cm-1, for temperatures ranging from 20 to 8000K. Our results demonstrate a good agreement with previous calculations for pure rotational transitions between low-lying rotational levels.

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However, we do find significant discrepancies for rovibrational processes involving highly-excited rotational and vibrational states. We attribute these differences to two key factors: 1) the broader range of intramolecular distances covered by ab initio points and 2) the superior accuracy of the PES, resulting from the utilization of the state-of-the-art quantum chemistry methods, compared to previous lower-level calculations.

Radiative transfer calculations performed with the new collisional data indicate that the population of rotational levels in excited vibrational states experiences significant modifications, highlighting the critical need for this updated dataset in models of high-temperature astrophysical environments.

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