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 and and distinguished by the way they interact. There are also three antineutrinos, and
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
).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.
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.
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.
11.
12.
R. S.
Raghavan
, S.
Pakvasa
, B. A.
Brown
, Phys. Rev. Lett.
57
, 1801
(1986
).13.
J. N.
Bahcall
, M.
Baldo‐Ceolin
, D. B.
Cline
, C.
Rubbia
, Phys. Lett. B
178
, 324
(1986
).14.
R. E.
Lanou
, H. J.
Maris
, G. M.
Seidel
, Phys. Rev. Lett.
58
, 2498
(1987
).See also L. Kadanoff, PHYSICS TODAY, August 1987, p. 7.
This content is only available via PDF.
© 1989 American Institute of Physics.
1989
American Institute of Physics
You do not currently have access to this content.
