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The Future of Solar Neutrinos

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arxiv 2107.08613 v1 pith:OMPW4S6A submitted 2021-07-19 hep-ph astro-ph.SRhep-exnucl-ex

classification hep-phastro-ph.SRhep-exnucl-ex
keywords solarreviewcurrentexperimentalfutureincludingstatediscuss
verification ladder T0 review T1 audit T2 compute T3 formal

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In this article we review the current state of the field of solar neutrinos, including flavour oscillations, non-standard effects, solar models, cross section measurements, and the broad experimental program thus motivated and enabled. We discuss the historical discoveries that contributed to current knowledge, and define critical open questions to be addressed in the next decade. We discuss the state of the art of standard solar models, including uncertainties and problems related to the solar composition, and review experimental and model solar neutrino fluxes, including future prospects. We review the state of the art of the nuclear reaction data relevant for solar fusion in the proton-proton chain and carbon-nitrogen-oxygen cycle. Finally, we review the current and future experimental program that can address outstanding questions in this field.

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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. Sensitivity of nEXO to $^{136}$Xe Charged-Current Interactions: Background-free Searches for Solar Neutrinos and Fermionic Dark Matter

    nucl-ex 2025-06 conditional novelty 6.0 of 10

    A new delayed-coincidence tag from 136Cs isomers could let the nEXO detector reject backgrounds down to 10^-9 and measure CNO solar neutrinos, the 7Be neutrino energy, and sub-MeV fermionic dark matter.

  2. Solar neutrinos

    hep-ph 2025-01 conditional novelty 1.0 of 10

    A concise pedagogical introduction to solar neutrino physics, from the standard solar model to neutrino oscillation and experimental achievements.

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