Bigravitational origin of dark matter

E Babichev, L Marzola, M Raidal, A Schmidt-May… - Physical Review D, 2016 - APS
E Babichev, L Marzola, M Raidal, A Schmidt-May, F Urban, H Veermäe, M von Strauss
Physical Review D, 2016APS
Observational evidence for dark matter is limited to gravitational effects. Dedicated searches
have yielded null results, challenging the most popular models. This can be explained if cold
dark matter is a massive spin-2 particle and, thus, a manifestation of gravity itself. In the
unique consistent theory for a massless and a massive spin-2 field, the latter can be heavy,
stable on cosmological scales, and produced with correct abundance, and its matter
coupling is naturally as weak as the gravitational one. The theory satisfies current gravity …
Observational evidence for dark matter is limited to gravitational effects. Dedicated searches have yielded null results, challenging the most popular models. This can be explained if cold dark matter is a massive spin-2 particle and, thus, a manifestation of gravity itself. In the unique consistent theory for a massless and a massive spin-2 field, the latter can be heavy, stable on cosmological scales, and produced with correct abundance, and its matter coupling is naturally as weak as the gravitational one. The theory satisfies current gravity tests, and we suggest several gravitational signatures.
American Physical Society
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