Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem

Details Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..69..717s&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 69, no. 5, Aug. 3, 1992, p. 717-720. Research supported by DOE, NSF, and NASA.

Statistics

Computation

50

Computational Astrophysics, Monte Carlo Method, Solar Neutrinos, Astronomical Models, Missing Mass (Astrophysics), Particle Flux Density

Scientific paper

The paper explores the impact of astrophysical uncertainties on the Mikheyev-Smirnov-Wolfenstein (MSW) solution by calculating the allowed MSW solutions for 1000 different solar models with a Monte Carlo selection of solar model input parameters, assuming a full three-family MSW mixing. Applications are made to the chlorine, gallium, Kamiokande, and Borexino experiments. The initial GALLEX result limits the mixing parameters to the upper diagonal and the vertical regions of the MSW triangle. The expected event rates in the Borexino experiment are also calculated, assuming the MSW solutions implied by GALLEX.

Affiliated with

Also associated with

No associations

Rating

Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Monte Carlo exploration of Mikheyev-Smirnov-Wolfenstein solutions to the solar neutrino problem will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1168801