Solar Neutrinos

Abstract

The status of the solar neutrino problem is reviewed. Attempts to explain the observed deficit and spectral distortion, both by astrophysical and particle physics methods, are described. It is argued that the comparison of all experiments strongly prefers the particle physics solutions.

Comments: Invited talk presented at 32nd International School of Subnuclear Physics, Erice, July 1994. 33 pages, Latex, 15 figures, not included; postscript file with embedded figures by anonymous ftp at ftp://dept.physics.upenn.edu/pub/Langacker/erice.ps