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Non-equilibrium h-2 formation in the early universe: energy exchanges, rate coefficients, and spectral distortions

Coppola, CM; D'Introno, R; Galli, D; Tennyson, J; Longo, S; (2012) Non-equilibrium h-2 formation in the early universe: energy exchanges, rate coefficients, and spectral distortions. Astrophysical Journal Supplement Series , 199 (1) , Article 16. 10.1088/0067-0049/199/1/16. Green open access

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Abstract

Energy exchange processes play a crucial role in the early universe, affecting the thermal balance and the dynamical evolution of the primordial gas. In the present work we focus on the consequences of a non-thermal distribution of the level populations of H2: first, we determine the excitation temperatures of vibrational transitions and the non-equilibrium heat transfer; second, we compare the modifications to chemical reaction rate coefficients with respect to the values obtained assuming local thermodynamic equilibrium; and third, we compute the spectral distortions to the cosmic background radiation generated by the formation of H2 in vibrationally excited levels. We conclude that non-equilibrium processes cannot be ignored in cosmological simulations of the evolution of baryons, although their observational signatures remain below current limits of detection. New fits to the equilibrium and non-equilibrium heat transfer functions are provided.

Type: Article
Title: Non-equilibrium h-2 formation in the early universe: energy exchanges, rate coefficients, and spectral distortions
Open access status: An open access version is available from UCL Discovery
DOI: 10.1088/0067-0049/199/1/16
Publisher version: http://dx.doi.org/10.1088/0067-0049/199/1/16
Language: English
Keywords: Cosmic background radiation, Early universe, Molecular processes
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/1334975
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