Neutrino masses and solar neutrinos
It has been pointed out by Bahcall and Bethe and others that all solar neutrino data can be explained by MSW oscillations with m({nu}{sub {mu}}) {approximately} 10{sup {minus}3} eV consistent with ideas grand unified theories (GUTS). There is a second possibility consistent with GUTS ideas with m({nu}{sub {tau}}) {approximately} 10{sup {minus}2} eV and m({nu} {sub {mu}}) {approximately} 10 {sup {minus}4} eV. The two cases can be distinguished by a measurement of the solar neutrinos from {sup {tau}}Be.
- Research Organization:
- Carnegie-Mellon Univ., Pittsburgh, PA (United States). Dept. of Physics
- Sponsoring Organization:
- USDOE, Washington, DC (United States)
- DOE Contract Number:
- FG02-91ER40682
- OSTI ID:
- 10187797
- Report Number(s):
- DOE/ER/40682--3; CMU-HEP--92-08; ON: DE93002416
- Country of Publication:
- United States
- Language:
- English
Similar Records
Neutrino masses and solar neutrinos
Neutrino masses and solar neutrinos
Right-handed-neutrino Majorana mass at the SUSY GUT scale and the solution of the solar-neutrino problem
Technical Report
·
Tue Dec 31 23:00:00 EST 1991
·
OSTI ID:6967046
Neutrino masses and solar neutrinos
Journal Article
·
Mon Jun 15 00:00:00 EDT 1992
· Physical Review, D (Particles Fields); (United States)
·
OSTI ID:7106183
Right-handed-neutrino Majorana mass at the SUSY GUT scale and the solution of the solar-neutrino problem
Journal Article
·
Fri Jul 01 00:00:00 EDT 1994
· Physical Review, D (Particles Fields); (United States)
·
OSTI ID:7112517