Solar models and solar neutrino oscillations

By J. Bahcall, C. Peña-Garay. 2004

149 citations recorded by the source corpus.

We provide a summary of the current knowledge, theoretical and experimental, of solar neutrino fluxes and of the masses and mixing angles that characterize solar neutrino oscillations. We also summarize the principal reasons for performing new solar neutrino experiments and what we anticipate from future studies.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/e5db97f94bd80c7fa68e0c7a358e5041045143e8

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Nuclear and High Energy Physics

1. H. M. Antia
2. Z. Xing
3. S. Basu
4. A. Serenelli
5. C. Giunti
6. F. Feruglio

Citations in the corpus

• Helioseismology and Solar Abundances (2007, methodology): “The effect of these uncertainties on neutrino fluxes has been discussed by Bahcall & Peña-Garay (2004), and Bahcall et al. (2006).”
• Flavor structures of charged fermions and massive neutrinos (2019, background): “In this case the distance-averaged probability of solar 8B neutrino oscillations reads [386]”