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Asymmetric Dark Matter · Around

2009

Asymmetric Dark Matter

Kaplan, David E., Luty, Markus A., Zurek, Kathryn M.

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We consider a simple class of models in which the relic density of dark matter is determined by the baryon asymmetry of the universe.

In these models a $B - L$ asymmetry generated at high temperatures is transfered to the dark matter, which is charged under $B - L$.
The interactions that transfer the asymmetry decouple at temperatures above the dark matter mass, freezing in a dark matter asymmetry of order the baryon asymmetry.
This explains the observed relation between the baryon and dark matter densities for dark matter mass in the range 5--15 GeV.

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