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A Dark-Disk Universe · Around

2013

A Dark-Disk Universe

Fan, JiJi, Katz, Andrey, Randall, Lisa et al.

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We point out that current constraints on dark matter imply only that the majority of dark matter is cold and collisionless.

A subdominant fraction of dark matter could have much stronger interactions.
In particular, it could interact in a manner that dissipates energy, thereby cooling into a rotationally-supported disk, much as baryons do.
We call this proposed new dark matter component Double-Disk Dark Matter (DDDM).

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