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High Energy Physics - Phenomenology

arXiv:1310.0823 (hep-ph)
[Submitted on 2 Oct 2013]

Title:Solar axion flux from the axion-electron coupling

Authors:Javier Redondo
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Abstract:In non-hadronic axion models, where axions couple to electrons at tree level, the solar axion flux is completely dominated by the ABC reactions (Atomic recombination and deexcitation, Bremsstrahlung and Compton). In this paper the ABC flux is computed from available libraries of monochromatic photon radiative opacities (OP, LEDCOP and OPAS) by exploiting the relations between axion and photon emission cross sections. These results turn to be ~ 30% larger than previous estimates due to atomic recombination (free-bound electron transitions) and deexcitation (bound-bound), which where not previously taken into account.
Comments: 24 pages, 9 figures. Data points for the solar-axion flux are provided in the file this http URL uploaded with the paper
Subjects: High Energy Physics - Phenomenology (hep-ph)
Report number: MPP-2011-219
Cite as: arXiv:1310.0823 [hep-ph]
  (or arXiv:1310.0823v1 [hep-ph] for this version)
  https://doi.org/10.48550/arXiv.1310.0823
Related DOI: https://doi.org/10.1088/1475-7516/2013/12/008

Submission history

From: Javier Redondo [view email]
[v1] Wed, 2 Oct 2013 20:00:04 UTC (1,240 KB)
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