Solar Neutrinos: Where We Are, What We Need

Details Solar Neutrinos: Where We Are, What We Need Solar Neutrinos: Where We Are, What We Need

1998-02-17

arxiv.org/abs/nucl-th/9802050v1

Nucl.Phys. A631 (1998) 29c-41c

Physics

Nuclear Physics

Nuclear Theory

20 pages, RevTeX file. To appear in the Proceedings of the 15th International Conference on Few-Body Problems in Physics, Gron

Scientific paper

10.1016/S0375-9474(98)00013-X

This talk compares standard model predictions with the results of solar neutrino experiments. Here `standard model' means the combined standard model of minimal electroweak theory plus a standard solar model. I emphasize the importance of recent analyses in which the neutrino fluxes are treated as free parameters, independent of any constraints from solar models, and the stunning agreement between the predictions of standard solar models and helioseismological measurements. In order to interpret solar neutrino experiments more accurately in terms of fundamental physics and astronomy, we need improved improved nuclear physics data. I describe the five most important nuclear physics problems whose solution is required for understanding the precise implications of solar neutrino experiments.

Affiliated with

Also associated with

No associations

Rating

Solar Neutrinos: Where We Are, What We Need 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 Solar Neutrinos: Where We Are, What We Need, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar Neutrinos: Where We Are, What We Need will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-602911