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Dark matter particles gravitationally trapped inside the Sun may annihilate into Standard Model particles, producing a flux of neutrinos.
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M. Cirelli, N. Fornengo, T. Montaruli, I. A. Sokalski, A. Strumia, et. al
2005
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F. Halzen and D. Hooper, Prospects for detecting dark matter with neutrino telescopes in light of recent results from direct detection experiments
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S. K. Agarwalla, Some aspects of neutrino mixing and oscillations · 2009
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2010
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LAGUNA Collaboration
2010
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PhD thesis, Glasgow university, 2010
A. Laing, Optimization of Detectors for the Golden Channel at a Neutrino Factory · 2010
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2010
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M. Blennow and E. Fernandez-Martinez, Neutrino oscillation parameter sampling with MonteCUBES
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https://webcast.stsci.edu/webcast/detail.xhtml?talkid=2426
“2011 may symposium on dark matter, space telescope science institute baltimore, maryland.” · 2011
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J. Jochum et. al
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L. M. Krauss, M. Srednicki, and F. Wilczek, Solar System Constraints and Signatures for Dark Matter Candidates
2083
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