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HeH+ Collisions with H2: Rotationally Inelastic Cross Sections and Rate Coefficients from Quantum Dynamics at

K Giri1, L González-Sánchez2, Rupayan Biswas3

  • 1Department of Computational Sciences, Central University of Punjab, Bathinda, Punjab 151401, India.

The Journal of Physical Chemistry. A
|April 1, 2022
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We developed an accurate potential energy surface for HeH+-H2 interactions. Hydrogen molecules (H2) are highly effective at exciting helium hydride ions (HeH+) in interstellar conditions.

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Area of Science:

  • Physical Chemistry
  • Chemical Physics
  • Computational Chemistry

Background:

  • Helium hydride ion (HeH+) is a key species in interstellar chemistry.
  • Understanding HeH+ interactions with other molecules is crucial for modeling interstellar environments.

Purpose of the Study:

  • To compute an accurate four-dimensional potential energy surface for the HeH+-H2 system.
  • To investigate the rotational excitation of HeH+ by H2 collisions at interstellar temperatures.

Main Methods:

  • Ab initio electronic structure calculations were performed.
  • An artificial neural network was used to fit the potential energy surface.
  • Quantum close coupling calculations were employed to determine state-to-state cross sections and rate coefficients.

Main Results:

  • Accurate four-dimensional potential energy surface for HeH+-H2 was generated.
  • Rate coefficients for HeH+ rotational excitation by H2 were computed for interstellar conditions.
  • H2 was identified as a highly efficient collision partner for exciting HeH+.

Conclusions:

  • Reduced-dimensionality calculations agree well with four-dimensional results for non-rotationally excited HeH+.
  • H2 is more effective than H or He in inducing rotational excitation of HeH+ at interstellar temperatures.
  • The findings highlight the importance of HeH+-H2 interactions in interstellar chemical kinetics.