A high-energy neutrino signature from supersymmetric relics

John S. Hagelin, K. W. Ng, Keith A. Olive

Research output: Contribution to journalArticlepeer-review

80 Scopus citations


We compute the energy spectrum of high-energy (0.1-10 GeV) neutrinos produced by the annihilation of supersymmetric (SUSY) cold dark matter trapped in the sun. We compare this spectrum to the spectrum of atmospheric neutrinos and find that in the direction of the sun the solar flux of neutrinos can exceed the atmospheric background for neutrino energies Eν {greater-than or approximate} 1 GeV, and are as much as a factor ∼ 30 above background for energies Eν ∼ few GeV. We discuss these signatures for standard SUSY relics as well as for superstring relics.

Original languageEnglish (US)
Pages (from-to)375-380
Number of pages6
JournalPhysics Letters B
Issue number4
StatePublished - Nov 20 1986

Bibliographical note

Funding Information:
We would like to thank D. Burke, S. Gasiorowicz, J. LoSecco, M. Srednicki and S. Rudaz for valuable discussions. The work of K.-W.N. and K.A.O. was supported in part by DOE grant DE-AC02-83ER-40105.


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