Systematic uncertainties from halo asphericity in dark matter searches
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Undergraduate course
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Elsevier B.V.
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Acesso aberto
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Abstract
Dark matter halos are predicted to be non-spherical by N-body simulations. Using data from the large N-body cosmological simulation Bolshoi, we quantify the systematic uncertainties due to halo asphericity on the determination of local dark matter density and the J factors for dark matter annihilations and decay from the galactic center.
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English
Citation
Nuclear And Particle Physics Proceedings. Amsterdam: Elsevier Science Bv, v. 267, p. 345-352, 2015.
