The effect of random matter density perturbations on the MSW solution to the solar neutrino problem
Authors:
- H. NunokawaHNH. Nunokawa
- A. RossiARA. Rossi
- V.B. SenlikozVSV.B. Senlikoz
- J.W.F. ValleJVJ.W.F. Valle
- 1 July 1996
- journal article
- Published by Elsevier in Nuclear Physics B
- Vol. 472 (3) , 495-517
Abstract
No abstract availableKeywords
All Related Versions
This publication has 28 references indexed in Scilit:
- Just-so oscillation: as just as MSW?Physics Letters B, 1996
- Vacuum oscillation solution to the solar neutrino problem in standard and nonstandard picturesPhysical Review D, 1995
- Two solar neutrino problemsPhysics Letters B, 1994
- Future solar neutrino spectroscopy and neutrino propertiesPhysics Letters B, 1994
- Astrophysical solutions are incompatible with the solar neutrino dataPhysical Review D, 1994
- The solar interiorPhysics Reports, 1993
- Toward a unified classical model of the sun - On the sensitivity of neutrinos and helioseismology to the microscopic physicsThe Astrophysical Journal, 1993
- Standard solar models, with and without helium diffusion, and the solar neutrino problemReviews of Modern Physics, 1992
- Solar models, neutrino experiments, and helioseismologyReviews of Modern Physics, 1988
- Resonance oscillations of neutrinos in matterSoviet Physics Uspekhi, 1987