Neutrino Oscillations and Solar Neutrinos

JUL 01, 1989

The hypothesized quantum mechanical process in which neutrinos transform from one ‘flavor’ into another can be studied by observing solar neutrinos with a new generation of highly sensitive detectors.

DOI: 10.1063/1.881173

Lincoln Wolfenstein

Eugene W. Beier

The neutrino is the elementary particle postulated by Wolfgang Pauli to account for the apparent nonconservation of energy in nuclear beta decay. Neutrinos are now believed to exist in at least three varieties, or “flavors,” labeled $ν_{e},$ $ν_{μ}$ and $ν_{τ}$ and distinguished by the way they interact. There are also three antineutrinos, ${ν̄}_{e},$ ${ν̄}_{μ}$ and ${ν̄}_{τ} .$

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References

1. S. Boris, A. Golutvin, L. Laptin, V. Lubimov, V. Nagovizin, E. Novikov, V. Nozik, V. Soloshenko, I. Tihomirov, E. Tretyakov, Phys. Lett. B. 159, 217 (1985).
2. M. Fritschi, E. Holzschuh, W. Kündig, J. W. Petersen, R. E. Pixley, H. Stüssi, Phys. Lett. B, 173, 485 (1986).https://doi.org/PYLBAJ
3. J. K. Rowley, B. T. Cleveland, R. Davis Jr, in Solar Neutrinos and Neutrino Astronomy, AIP Conf. Proc. 126, M. L. Cherry, W. Fowler, K. Lande, eds., AIP, New York (1985), p. 1.
4. J. N. Bahcall, R. K. Ulrich, Rev. Mod. Phys. 60, 297 (1988).https://doi.org/RMPHAT
5. M. J. Newman, Physics of the Sun, vol. 3, P. A. Sturrock, T. E. Holzer, D. M. Mihalas, R. K. Ulrich, eds., Reidel, Dordrecht, The Netherlands (1986), p. 33.
6. R. Davis Jr, K. Lande, B. T. Cleveland, J. Ullman, J. K. Rowley, in Proceedings of Neutrino ’88, J. Schneps, ed., World Scientific, Singapore (1989), to be published.
7. M. B. Voloshin, M. I. Vysotsky, L. B. Okun, Zh. Eksp. Teor. Fiz. 91, 754 (1986) https://doi.org/ZETFA7
[M. B. Voloshin, M. I. Vysotsky, L. B. Okun, Sov. Phys. JETP 64, 446 (1986)].https://doi.org/SPHJAR
8. K. S. Hirata et al., Phys. Rev. Lett. (3 July 1989), in press.
See also M. Koshiba, PHYSICS TODAY, December 1987, p. 38.
9. M. Gell‐Mann, P. Ramond, R. Slansky, in Supergravity, P. van Nieuwenhuizen, D. Freedman, eds., North‐Holland, Amsterdam (1979), p. 315.
10. S. P. Mikheyev, A. Yu. Smirnov, Nuovo Cimento C 9, 17 (1986).
L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).https://doi.org/PRVDAQ
11. S. P. Rosen, J. M. Gelb, Phys. Rev. D 34, 969 (1986).https://doi.org/PRVDAQ
12. R. S. Raghavan, S. Pakvasa, B. A. Brown, Phys. Rev. Lett. 57, 1801 (1986).https://doi.org/PRLTAO
13. J. N. Bahcall, M. Baldo‐Ceolin, D. B. Cline, C. Rubbia, Phys. Lett. B 178, 324 (1986).https://doi.org/PYLBAJ
14. R. E. Lanou, H. J. Maris, G. M. Seidel, Phys. Rev. Lett. 58, 2498 (1987). https://doi.org/PRLTAO
See also L. Kadanoff, PHYSICS TODAY, August 1987, p. 7.

More about the authors

Lincoln Wolfenstein, Carnegie Mellon University, Pittsburgh.

Eugene W. Beier, University of Pennsylvania, Philadelphia.