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Neutrino Mass and New Physics

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arxiv hep-ph/0603118 v2 pith:3F4SB3BU submitted 2006-03-16 hep-ph

Neutrino Mass and New Physics

classification hep-ph
keywords flavorneutrinosphysicsdiscussleptonsneutrinoproblemquarks
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We review the present state of and future outlook for our understanding of neutrino masses and mixings. We discuss what we think are the most important perspectives on the plausible and natural scenarios for neutrinos and what may have the most promise to throw light on the flavor problem of quarks and leptons. We focus on the seesaw mechanism which fits into the big picture of particle physics such as supersymmetry and grand unification providing a unified approach to flavor problem of quarks and leptons. We argue that in combination with family symmetries, this may be at the heart of a unified understanding of flavor puzzle. We also discuss other new physics ideas such as neutrinos in models with extra dimensions and possible theoretical implications of sterile neutrinos. We outline some tests for the various schemes.

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Cited by 4 Pith papers

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

  1. Self-interacting neutrinos in cosmological perturbation theory -- integrating the collision kernel

    astro-ph.CO 2026-06 unverdicted novelty 7.0

    Derives exact rational-plus-π² closed forms for every multipole coefficient α_ℓ in the neutrino collision kernel by rewriting the kernel as angular derivatives of a Yukawa potential and reducing the integrals via a fi...

  2. Are neutrinos Majorana? Fixed-target and high-energy astrophysical searches decide

    hep-ph 2026-06 unverdicted novelty 6.0

    Correlated HNL discovery at SHiP and flavor ratio shifts in astrophysical neutrinos at telescopes would establish neutrinos as Majorana fermions.

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

    hep-ph 2026-01 conditional novelty 5.0

    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.

  4. Cosmological searches for the neutrino mass scale and mass ordering

    astro-ph.CO 2019-07 unverdicted novelty 4.0

    Thesis summarizing an upper limit of 0.12 eV on the neutrino mass sum, bias calibration via CMB lensing cross-correlations, and tighter limits plus stronger normal-ordering preference in non-phantom dynamical dark ene...