Solar axion flux from the axion-electron coupling

By J. Redondo. 2013

162 citations recorded by the source corpus.

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.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/13bad4fd5d5a5ec87333f60c0d8502e9000f1963

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In Nuclear and High Energy Physics

  1. J. Redondo
  2. Igor G. Irastorza
  3. A. Ringwald
  4. Maurizio Giannotti
  5. K. Saikawa
  6. S. Basu
  7. A. Serenelli
  8. G. Raffelt

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