Cosmic quarkonium: A probe of dark matter

Mark Srednicki, Stefan Theisen, and Joseph Silk
Phys. Rev. Lett. 56, 263 – Published 20 January 1986; Erratum Phys. Rev. Lett. 56, 1883 (1986)
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Abstract

If our galactic halo is composed of heavy (several gigaelectron- volts), weakly interacting particles, pair annihilation into a heavy-quarkantiquark bound state plus a monochromatic photon can produce potentially observable sharp peaks in the diffuse cosmic-γ-ray background.

  • Received 20 November 1985

DOI:https://doi.org/10.1103/PhysRevLett.56.263

©1986 American Physical Society

Erratum

Cosmic Quarkonium: A Probe of Dark Matter.

Mark Srednicki, Stefan Theisen, and Joseph Silk
Phys. Rev. Lett. 56, 1883 (1986)

Authors & Affiliations

Mark Srednicki and Stefan Theisen

  • Department of Physics, University of California, Santa Barbara, California 93106

Joseph Silk

  • Department of Astronomy, University of California, Berkeley, California 94720

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Vol. 56, Iss. 3 — 20 January 1986

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