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Neutrinos in cosmology

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arxiv hep-ph/0202122 v2 pith:FQVWUO75 submitted 2002-02-13 hep-ph astro-ph

A.D. Dolgov This is my paper · ORCID
classification hep-phastro-ph
keywords neutrinoscosmologicalneutrinouniversecosmiclargesubjectsasymmetry
verification ladder T0 review T1 audit T2 compute T3 formal
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Cosmological implications of neutrinos are reviewed. The following subjects are discussed at a different level of scrutiny: cosmological limits on neutrino mass, neutrinos and primordial nucleosynthesis, cosmological constraints on unstable neutrinos, lepton asymmetry of the universe, impact of neutrinos on cosmic microwave radiation, neutrinos and the large scale structure of the universe, neutrino oscillations in the early universe, baryo/lepto-genesis and neutrinos, neutrinos and high energy cosmic rays, and briefly some more exotic subjects: neutrino balls, mirror neutrinos, and neutrinos from large extra dimensions.

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Cited by 4 Pith papers

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

  1. Overdamping of Neutron-Mirror-Neutron Transitions in Neutron Stars

    hep-ph 2026-03 conditional novelty 6.5 of 10

    Collisional decoherence overdamps n–n′ transitions in neutron stars, yielding Γ ≈ 4ε²/M ≪ oscillation rates and a mirror admixture suppressed by ~4ε²/M² at all times.

  2. Pathways and impediments towards a detection of the relic neutrino wind

    hep-ph 2026-07 accept novelty 6.0 of 10

    Detecting the cosmic neutrino background's dipole anisotropy via tritium capture requires ~10^5 times the exposure needed for flux detection, with Majorana neutrinos suffering an additional (m_ν/T_ν)^2 suppression.

  3. Enlightening dark moments of neutrino with superradiance

    hep-ph 2026-08 conditional novelty 5.0 of 10

    Quenched superradiance of dark photon clouds around spinning primordial black holes could turn neutrino electromagnetic moment bounds into observable neutrino fluxes and limits on PBH abundance.

  4. Another relation among the neutrino mass-squared differences?

    hep-ph 2026-01 conditional novelty 5.0 of 10

    The ratio (√Δm²31 + √Δm²21)/(√Δm²31 − √Δm²21) is claimed to be exactly √2, implying m1 ≈ 0 and absolute neutrino masses near 0.009 eV and 0.050 eV.

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