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2014

Diurnal modulation signal from dissipative hidden sector dark matter

Foot, R., Vagnozzi, S.

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We consider a simple generic dissipative dark matter model: a hidden sector featuring two dark matter particles charged under an unbroken $U(1)'$ interaction.

Previous work has shown that such a model has the potential to explain dark matter phenomena on both large and small scales.
In this framework, the dark matter halo in spiral galaxies features nontrivial dynamics, with the halo energy loss due to dissipative interactions balanced by a heat source.
Ordinary supernovae can potentially supply this heat provided kinetic mixing interaction exists with strength $\epsilon \sim 10^{-9}$.

Diurnal modulation signal from dissipative hidden sector dark matter · Around

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