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Neutrino physics and the mirror world: how exact parity symmetry explains the solar neutrino deficit, the atmospheric neutrino anomaly and the LSND experiment

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arxiv hep-ph/9505359 v2 pith:G3WGNOAE submitted 1995-05-23 hep-ph astro-ph

classification hep-phastro-ph
keywords neutrinosymmetryanomaliesmodelparityphysicsanomalyatmospheric
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abstract

Evidence for $\bar \nu_{\mu} \rightarrow \bar \nu_e$ oscillations has been reported at LAMPF using the LSND detector. Further evidence for neutrino mixing comes from the solar neutrino deficit and the atmospheric neutrino anomaly. All of these anomalies require new physics. We show that all of these anomalies can be explained if the standard model is enlarged so that an unbroken parity symmetry can be defined. This explanation holds independently of the actual model for neutrino masses. Thus, we argue that parity symmetry is not only a beautiful candidate for a symmetry beyond the standard model, but it can also explain the known neutrino physics anomalies.

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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. Universal Seesaw Pati-Salam Model with P for Strong CP

    hep-ph 2025-12 conditional novelty 6.0 of 10

    A parity-symmetric Pati-Salam model with universal seesaw masses gives an axionless strong-CP solution and radiatively induced neutrino masses.

  2. Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit?

    astro-ph.CO 2026-06 unverdicted novelty 5.0 of 10

    Cosmological observations constrain the effective abundance of light sterile neutrinos tightly while allowing non-fully-thermalized realizations to remain viable across LambdaCDM and CPL models.

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