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Solar neutrinos

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arxiv 2501.09971 v1 pith:WXSO5F25 submitted 2025-01-17 hep-ph astro-ph.SRhep-exnucl-ex

classification hep-phastro-ph.SRhep-exnucl-ex
keywords solarneutrinoneutrinososcillationphysicsabundantlyachievementsactive
verification ladder T0 review T1 audit T2 compute T3 formal
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Solar neutrinos, generated abundantly by thermonuclear reactions in the solar interior, offer a unique tool for studying astrophysics and particle physics. The observation of solar neutrinos has led to the discovery of neutrino oscillation, a topic currently under active research, and it has been recognized by two Nobel Prizes. In this pedagogical introduction to solar neutrino physics, we will guide readers through several key questions: How are solar neutrinos produced? How are they detected? What is the solar neutrino problem, and how is it resolved by neutrino oscillation? This article also presents a brief overview of the theory of solar neutrino oscillation, the experimental achievements, new physics relevant to solar neutrinos, and the prospects in this field.

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Cited by 1 Pith paper

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

  1. FCL-COD: Weakly Supervised Camouflaged Object Detection with Frequency-aware and Contrastive Learning

    cs.CV 2026-03 unverdicted novelty 5.0 of 10

    FCL-COD adapts SAM with frequency-aware LoRA and gradient-aware contrastive learning and claims to outperform both weakly and fully supervised camouflaged object detectors on three benchmarks.

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