Neutrino Propagation Through Helioseismic Waves

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

27 pages, plain TeX, 10 figures

Scientific paper

10.1016/S0550-3213(97)00672-X

Motivated by earlier calculations showing large effects when neutrinos propagate through fluctuating media, we perform here a detailed analysis of how density fluctuations in the sun in the form of helioseismic waves can modify the MSW solution to the solar neutrino problem. We find negligible effects for the MSW spectrum, even under extreme circumstances. There are two main reasons why our conclusions differ from earlier analyses. First, most helioseismic waves do not affect neutrino propagation because their amplitude is too small in the MSW resonance region, which is the only region to whose fluctuations neutrinos are sensitive. There is one class of waves which may be subject to an instability, however, and so can have significantly larger amplitudes. But the wavelength for these waves is so long that it invalidates the previous methods of calculation. Our more complete calculation significantly reduces the prediction for their influence on neutrino propagation.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Neutrino Propagation Through Helioseismic Waves 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 Neutrino Propagation Through Helioseismic Waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino Propagation Through Helioseismic Waves will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-151379

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.