Self-interacting dark matter constraints in a thick dark disk scenario

被引:3
作者
Vattis, Kyriakos [1 ]
Koushiappas, Savvas M. [1 ]
机构
[1] Brown Univ, Dept Phys, 182 Hope St, Providence, RI 02912 USA
关键词
COSMOLOGICAL SIMULATIONS; MILKY-WAY; SOLAR; DENSITY; MODELS;
D O I
10.1103/PhysRevD.97.103003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A thick dark matter disk is predicted in cold dark matter simulations as the outcome of the interaction between accreted satellites and the stellar disk in Milky Way-sized halos. We study the effects of a self-interacting thick dark disk on the energetic neutrino flux from the Sun. We find that for particle masses between 100 GeV and 1 TeV and dark matter annihilation to tau(+)tau(-), either the self-interaction may not be strong enough to solve the small-scale structure motivation or a dark disk cannot be present in the Milky Way.
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页数:7
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