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Flavoring Monochromatic Neutrino Flux from Dark Matter Annihilation · Around

2011

Flavoring Monochromatic Neutrino Flux from Dark Matter Annihilation

Farzan, Yasaman

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As is well-known, if the scattering cross section of the Dark Matter (DM) particles off the nuclei inside the Sun is large enough, the Sun can trap DM particles.

In principle, the annihilation of DM pair inside the Sun can then lead to the detection of a relatively large flux of neutrinos in the neutrino telescopes.
If the annihilation directly produces a neutrino pair, the flux of neutrinos on Earth will be monochromatic.
In this case, the oscillatory terms in the oscillation probability lead to a novel seasonal variation of detected events which is sensitive to the initial flavor composition.

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Then

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V. Barger, Y. Gao, D. Marfatia, [arXiv:1109.5748 [hep-ph]]; see also, S. Razzaque and A. Y. Smirnov, JHEP 1107
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