Neutrino oscillations in matter
Reviews of Modern Physics, ISSN: 0034-6861, Vol: 61, Issue: 4, Page: 937-979
1989
- 517Citations
- 73Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
Citation Benchmarking is provided by Scopus and SciVal and is different from the metrics context provided by PlumX Metrics.
Article Description
Nonzero neutrino masses would provide new, unique information on particle physics beyond the standard model. Neutrino flavor oscillations provide the most sensitive method for directly testing for small neutrino masses. When the oscillations occur in matter, a resonance can occur that dramatically enhances the flavor mixing and can lead to conversion from one neutrino flavor to another. This is an attractive solution to the long-standing "solar neutrino problem." The phenomenon of neutrino oscillations in matter is reviewed. Analytic descriptions of the neutrino flavor survival probability in matter are considered in detail. A discussion is given for applications of neutrino oscillations in matter for the sun, Earth, supernovae, and the early universe. © 1989 The American Physical Society.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=33744746004&origin=inward; http://dx.doi.org/10.1103/revmodphys.61.937; https://link.aps.org/doi/10.1103/RevModPhys.61.937; http://harvest.aps.org/v2/journals/articles/10.1103/RevModPhys.61.937/fulltext; http://link.aps.org/article/10.1103/RevModPhys.61.937
American Physical Society (APS)
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