Helioseismic constraints on the solar neutrino fluxes

Details Helioseismic constraints on the solar neutrino fluxes Helioseismic constraints on the solar neutrino fluxes

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001esasp.464..491v&link_type=abstract

In: Proceedings of the SOHO 10/GONG 2000 Workshop: Helio- and asteroseismology at the dawn of the millennium, 2-6 October 2000,

Astronomy and Astrophysics

Astrophysics

Helioseismology, Solar Neutrinos

Scientific paper

Solar models are more and more constrained by helioseismology. Meanwhile, solar neutrino measurements at the earth are more and more precise owing to the various detectors working simultaneously. The astrophysical solutions to the solar neutrino problem which have been proposed in the past are ruled out and neutrino oscillations seem the most promising explanation for the observed spectrum. However the situation is not yet completely settled, either in astrophysics or in particle physics.

Affiliated with

Also associated with

No associations

Rating

Helioseismic constraints on the solar neutrino fluxes 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 Helioseismic constraints on the solar neutrino fluxes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Helioseismic constraints on the solar neutrino fluxes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-923623