Hostname: page-component-7bb8b95d7b-nptnm Total loading time: 0 Render date: 2024-09-19T23:45:19.991Z Has data issue: false hasContentIssue false

Neutrino Masses and Mixing

Published online by Cambridge University Press:  26 May 2016

Yoji Totsuka*
Affiliation:
KEK, High Energy Accelerator Research Organization, 1-1 Oho, Tsukuba, Ibaraki, 305-0801 Japan

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent results on neutrino masses and mixing are presented. There is convincing evidence for nonzero but tiny masses of at least two flavor neutrinos, based on two types of neutrino oscillations, solar and atmospheric neutrinos. The large mixing angle between first and second flavors and also the one between the second and third flavors were found, quite contrary to small mixing angles among quark flavors, and pose a new mystery.

Type
Part 10 Non-Photon Astrophysics and the Future
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Abdurashitov, J. N. et al. 2002, astro-ph/0204245 Google Scholar
Altmann, M. et al. 2000, Phys. Lett. B, 490, 16 Google Scholar
Bahcall, J. N., Pinsonneault, M. H., & Basu, S. 2001, ApJ, 555, 990 Google Scholar
Barr, G., et al. 1998, Phys. Rev. D, 39, 3532 Google Scholar
Cleveland, B. T. et al. 1998, ApJ, 496, 505 Google Scholar
Honda, M. et al. 1990, Phys. Lett. B, 248, 193 CrossRefGoogle Scholar
Kasuga, S. et al. 1996, Phys. Lett. B, 374, 238 Google Scholar
Langacker, P. 1983, Phys. Rev. D, 52, 4985 Google Scholar
Super-K, Collaboration 1998, Phys. Rev. Lett., 81, 1562 Google Scholar
Super-K, Collaboration 2001, Phys. Rev. Lett., 86, 5651 Google Scholar
SNO, Collaboration 2002, Phys. Rev. Lett., 89, 011301 Google Scholar
SNO, Collaboration, 2002a, Phys. Rev. Lett., 89, 011302 Google Scholar