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Implications of new GALLEX results for the Mikheyev-Smirnov-Wolfenstein solution of the solar neutrino problem

Journal Article · · Physical Review Letters; (United States)
 [1]; ;  [2]
  1. NASA/Fermilab Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, Illinois 60510 (United States)
  2. Department of Physics, The University of Texas at Arlington, Arlington, Texas 76019 (United States)

We compare the implications for {sup 7}Be and {ital pp} neutrinos of the two Mikheyev-Smirnov-Wolfenstein fits to the new GALLEX solar neutrino measurements. Small-mixing-angle solutions tend to suppress the former as electron neutrinos, but not the latter, and large-angle solutions tend to reduce both by about a factor of 2. The consequences for BOREXINO and similar solar neutrino-electron scattering experiments are discussed.

DOE Contract Number:
FG05-92ER40691
OSTI ID:
7199607
Journal Information:
Physical Review Letters; (United States), Journal Name: Physical Review Letters; (United States) Vol. 69:13; ISSN PRLTA; ISSN 0031-9007
Country of Publication:
United States
Language:
English