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arXiv · 1604.08564

Gravitational Origin of Dark Matter

Eugeny Babichev·Luca Marzola·Martti Raidal·Angnis Schmidt-May·Federico Urban·Hardi Veermäe·Mikael von Strauss
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Abstract

Observational evidence for the existence of Dark Matter is limited to its gravitational effects. The extensive program for dedicated searches has yielded null results so far, challenging the most popular models. Here we propose that this is the case because the very existence of cold Dark Matter is a manifestation of gravity itself. The consistent bimetric theory of gravity, the only known ghost-free extension of General Relativity involving a massless and a massive spin-2 field, automatically contains a perfect Dark Matter candidate. We demonstrate that the massive spin-2 particle can be heavy, stable on cosmological scales, and that it interacts with matter only through a gravitational type of coupling. Remarkably, these features persist in the same region of parameter space where bimetric theory satisfies the current gravity tests. We show that the observed Dark Matter abundance can be generated via freeze-in and suggest possible particle physics and gravitational signatures of our bimetric Dark Matter model.

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Eugeny Babichev, Luca Marzola, Martti Raidal, Angnis Schmidt-May, Federico Urban, Hardi Veermäe, Mikael von Strauss. 2016-04-28. Gravitational Origin of Dark Matter. https://doi.org/10.1103/physrevd.94.084055

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