Gamma-Ray Constraint on Galactic Positron Production by MeV Dark Matter

John F. Beacom, Nicole F. Bell, and Gianfranco Bertone
Phys. Rev. Lett. 94, 171301 – Published 5 May 2005

Abstract

The Galactic positrons, as observed by their annihilation gamma-ray line at 0.511 MeV, are difficult to account for with astrophysical sources. It has been proposed that they are produced instead by dark matter annihilation or decay in the inner Galactic halo. To avoid other constraints, these processes are required to occur “invisibly,” such that the eventual positron annihilation is the only detectable signal. However, electromagnetic radiative corrections to these processes inevitably produce real gamma rays (“internal bremsstrahlung”); this emission violates COMPTEL and EGRET constraints unless the dark matter mass is less than about 20 MeV.

  • Figure
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  • Received 16 September 2004

DOI:https://doi.org/10.1103/PhysRevLett.94.171301

©2005 American Physical Society

Authors & Affiliations

John F. Beacom1,2, Nicole F. Bell3,4, and Gianfranco Bertone3

  • 1Department of Physics, The Ohio State University, Columbus, Ohio 43210, USA
  • 2Department of Astronomy, The Ohio State University, Columbus, Ohio 43210, USA
  • 3NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510-0500, USA
  • 4Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California 91125, USA

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Issue

Vol. 94, Iss. 17 — 6 May 2005

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