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Neutrino physics from precision cosmology

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arxiv 1007.0658 v2 pith:W5SNUYDU submitted 2010-07-05 hep-ph astro-ph.CO

Steen Hannestad This is my paper
classification hep-phastro-ph.CO
keywords neutrinocosmologicalcosmologyphysicspropertiesaspectscurrentdetail
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Cosmology provides an excellent laboratory for testing various aspects of neutrino physics. Here, I review the current status of cosmological searches for neutrino mass, as well as other properties of neutrinos. Future cosmological probes of neutrino properties are also discussed in detail.

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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. Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy

    astro-ph.CO 2026-01 conditional novelty 6.0 of 10

    A combined-analysis of DESI galaxy clustering, CMB lensing, BAO, CMB, and supernovae yields percent-level Lambda-CDM parameters, improved dark-energy figure-of-merit, and neutrino-mass bounds that disfavor the inverte...

  2. Cosmological neutrino mass: a frequentist overview in light of DESI

    astro-ph.CO 2025-07 accept novelty 6.0 of 10

    A frequentist profile-likelihood analysis of DESI, Planck, ACT, and eBOSS Lyman-alpha data yields Σmν < 53 meV (95% C.L.) in flat ΛCDM and a CMB-independent bound of 285 meV.

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