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Emission of photons and relativistic axions from axion stars

Eric Braaten, Abhishek Mohapatra, and Hong Zhang
Phys. Rev. D 96, 031901(R) – Published 15 August 2017

Abstract

The number of nonrelativistic axions can be changed by inelastic reactions that produce photons or relativistic axions. Any odd number of axions can annihilate into two photons. Any even number of nonrelativistic axions can scatter into two relativistic axions. We calculate the rate at which axions are lost from axion stars from these inelastic reactions. In dilute systems of axions, the dominant inelastic reaction is axion decay into two photons. In sufficiently dense systems of axions, the dominant inelastic reaction is the scattering of four nonrelativistic axions into two relativistic axions. The scattering of odd numbers of axions into two photons produces monochromatic radio-frequency signals at odd-integer harmonics of the fundamental frequency set by the axion mass. This provides a unique signature for dense systems of axions, such as a dense axion star or a collapsing dilute axion star.

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  • Received 16 September 2016

DOI:https://doi.org/10.1103/PhysRevD.96.031901

© 2017 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Particles & Fields

Authors & Affiliations

Eric Braaten*, Abhishek Mohapatra, and Hong Zhang

  • Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA

  • *braaten@mps.ohio-state.edu
  • mohapatra.16@buckeyemail.osu.edu
  • zhang.5676@osu.edu

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Issue

Vol. 96, Iss. 3 — 1 August 2017

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