• Open Access

Gamma rays from dark mediators in white dwarfs

M. Cermeño and M. A. Pérez-García
Phys. Rev. D 98, 063002 – Published 5 September 2018

Abstract

We consider self-annihilation of dark matter, χ, into metastable mediators, Y, and their subsequent decay into photons inside white dwarfs. We focus on reactions of the type χχ¯YY, where mediators, besides having a finite decay lifetime at rest τrest1s, may suffer energy loss in the medium before they decay into photons, Yγγ. We obtain attenuated gamma-ray luminosities arising from the combination of both effects. Using complementary sets of astrophysical measurements from cold white dwarfs in the M4 globular cluster as well as direct and indirect dark matter searches, we discuss further constraints on dark mediator lifetimes.

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  • Received 9 July 2018

DOI:https://doi.org/10.1103/PhysRevD.98.063002

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

M. Cermeño* and M. A. Pérez-García

  • Department of Fundamental Physics, University of Salamanca, Plaza de la Merced s/n, E-37008 Salamanca, Spain

  • *marinacgavilan@usal.es
  • mperezga@usal.es

Article Text

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Issue

Vol. 98, Iss. 6 — 15 September 2018

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