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Spin-2 dark matter from anisotropic Universe in bigravity

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arxiv 2211.15873 v1 pith:3LZQKIXJ submitted 2022-11-29 gr-qc astro-ph.COhep-ph

classification gr-qcastro-ph.COhep-ph
keywords darkmatterbigravityspin-2fixedanisotropicgeneralpoint
verification ladder T0 review T1 audit T2 compute T3 formal
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Bigravity is one of the natural extensions of general relativity and contains an additional massive spin-2 field which can be a good candidate for dark matter. To discuss the production of spin-2 dark matter, we study fixed point solutions of the background equations for axisymmetric Bianchi type-I Universes in two bigravity theories without Boulware-Deser ghost, i.e., Hassan-Rosen bigravity and Minimal Theory of Bigravity. We investigate the local and global stability of the fixed points and classify them. Based on the general analysis, we propose a new scenario where spin-2 dark matter is produced by the transition from an anisotropic fixed point solution to isotropic one. The produced spin-2 dark matter can account for all or a part of dark matter and can be directly detected by laser interferometers in the same way as gravitational waves.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Massive graviton dark matter searches with long-baseline atom interferometers

    hep-ph 2024-12 conditional novelty 6.0 of 10

    Long-baseline atom interferometers could detect ultra-light spin-2 dark matter through three coupling channels, reaching mass and coupling ranges that LIGO and LISA cannot cover.

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