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Indirect searches for signatures of corpuscular dark matter have been performed using all cosmic messengers: gamma rays, cosmic rays, and neutrinos.
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Y. Ascasibar, P. Jean, C. Boehm and J. Knoedlseder, Constraints on dark matter and the shape of the Milky Way dark halo from the 511-keV line , Mon. Not. Roy. Astron. Soc. 368
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C. Giunti and C. W. Kim, Fundamentals of Neutrino Physics and Astrophysics . 4, 2007
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C. Boehm, Y. Farzan, T. Hambye, S. Palomares-Ruiz and S. Pascoli, Is it possible to explain neutrino masses with scalar dark matter? , Phys. Rev. D77
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2014
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2015
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R. Catena, Dark matter signals at neutrino telescopes in effective theories , JCAP 1504
2015
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C. A. Argüelles, J. Salvado and C. N. Weaver, “ ν \nu -SQuIDS.” https://github.com/Arguelles/nuSQuIDS , 2015
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Super-Kamiokande
2017
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2017
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R. Catena, WIMP capture and annihilation in the Earth in effective theories , JCAP 01
2017
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Particle Data Group
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I. Esteban, M. C. Gonzalez-Garcia, A. Hernandez-Cabezudo, M. Maltoni and T. Schwetz, “NuFIT.” NuFIT4.1(2019),www.nu-fit.org , 2019
2019
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2019
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10.5281/zenodo.3959654
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