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2019

Real Scalar Dark Matter: Relativistic Treatment

Arcadi, Giorgio, Lebedev, Oleg, Pokorski, Stefan et al.

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A stable real scalar provides one of the simplest possibilities to account for dark matter.

We consider the regime where its coupling to the Standard Model fields is negligibly small.
Due to self-coupling, the scalar field can reach thermal or at least kinetic equilibrium, in which case the system is characterized by its temperature and effective chemical potential.
We perform a fully relativistic analysis of dark matter evolution, thermalization conditions and different freeze-out regimes, including the chemical potential effects.

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