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Dark Matter Candidates - Axions, Neutralinos, Gravitinos, and Axinos

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arxiv 0811.3347 v1 pith:3UY3WZSU submitted 2008-11-20 hep-ph astro-phhep-ex

classification hep-phastro-phhep-ex
keywords darkmattercandidatesexperimentalmodelstandardappearastrophysical
verification ladder T0 review T1 audit T2 compute T3 formal

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The existence of dark matter provides strong evidence for physics beyond the Standard Model. Extending the Standard Model with the Peccei-Quinn symmetry and/or supersymmetry, compelling dark matter candidates appear. For the axion, the neutralino, the gravitino, and the axino, I review primordial production mechanisms, cosmological and astrophysical constraints, experimental searches, and prospects for experimental identification.

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Cited by 2 Pith papers

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

  1. Active galactic nuclei through the prism of galaxy clusters: bounds on axion-like particles

    astro-ph.HE 2025-06 conditional novelty 6.0 of 10

    Stacked gamma-ray spectra of 29 AGN-cluster pairs place new bounds on axion-like particles with masses around 1 to 10 neV, improving previous limits by up to a factor of four under the assumed cluster magnetic fields.

  2. The Heavy Gluino in Natural No-Scale $\cal{F}$-$SU$(5)

    hep-ph 2019-08 conditional novelty 5.0 of 10

    Relaxing the relic density constraint lets no-scale Flipped SU(5) push the gluino mass up to about 7.5 TeV, with the top quark mass and Higgs mass tradeoff setting the boundary.

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