Solar Models and Solar Neutrinos: Current Status
arXiv:hep-ph/0412068 · doi:10.1088/0031-8949/2005/T121/006
Abstract
I provide a summary of the current theoretical knowledge of solar neutrino fluxes as derived from precise solar models.
Neutrino Physics, Proceedings of the Nobel Symposium 2004, Enkoping, Sweden, August 19-24, 2004. Eds. L. Bergstrom, O. Botner, P. Carlson, P.O. Hulth & T. Ohlsson
References in corpus (8)
- Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
- What do we (not) know theoretically about solar neutrino fluxes?
- Helioseismological Implications of Recent Solar Abundance Determinations
- Constraining solar abundances using helioseismology
- Precise measurement of the ^7Be(p,gamma)^8B S-factor
- Three-Neutrino Mixing after the First Results from K2K and KamLAND
- Neutrinoless Double Beta Decay in Light of SNO Salt Data
- Sudbury Neutrino Observatory Results
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- Axion emission from nuclear magnetic dipole transitions
- Radioactivities in Low- and Intermediate-Mass Stars
- Neutrino astronomy and gamma-ray bursts
- Sub-stellar engulfment by a main sequence star: where is the lithium?
- Status and Perspectives of Astroparticle Physics in Europe
- On the angular distribution of IceCube high-energy events