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Symmetries and Algebraic Methods in Neutrino Physics

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arxiv 1809.02539 v1 pith:UGYGKDTJ submitted 2018-09-07 hep-ph astro-ph.SRnucl-th

A.B. Balantekin This is my paper · ORCID
classification hep-phastro-ph.SRnucl-th
keywords neutrinosymmetriesalgebraicassociatedastrophysicsbackgroundchosencollective
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Symmetry properties associated with neutrino propagation with or without a background of other particles, including neutrinos, is reviewed. The utility of symmetries is illustrated with examples chosen from the see-saw mechanism and both matter-enhanced and collective neutrino oscillations. The role of symmetries in neutrino astrophysics is highlighted.

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  1. Improved Approximations for Collective Neutrino Oscillations

    hep-ph 2026-07 conditional novelty 6.0 of 10

    Second-order BBGKY truncation of an su(n) one-plus-two-body Hamiltonian approximates collective neutrino dynamics beyond mean field at polynomial classical cost and reveals large-N phase and entanglement structure.

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