Electron-neutrino dynamics in a supernova and constraints on the electron-neutrino magnetic moment

Details Electron-neutrino dynamics in a supernova and constraints on the electron-neutrino magnetic moment Electron-neutrino dynamics in a supernova and constraints on the electron-neutrino magnetic moment

May 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pzetf..47..421v&link_type=abstract

Pis'ma v Zhurnal Eksperimental'noi i Teoreticheskoi Fiziki (ISSN 0370-274X), vol. 47, May 10, 1988, p. 421-423. In Russian.

Physics

3

Magnetic Moments, Solar Neutrinos, Stellar Magnetic Fields, Supernova 1987A, Electron Energy, Stellar Cores, Stellar Mass Ejection

Scientific paper

It is shown that, if an electron neutrino has a magnetic moment mu of about 10 to the -11th mu(B), a resonant total reversal of its spirality can arise in the nuclear layer of a supernova having a density of 10 to the -12th g/cu cm. Therefore, contrary to assertions made in the literature, this value of mu not only does not contradict SN 1987A neutrino data but can explain the supernova shell ejection mechanism.

Affiliated with

Also associated with

No associations

Rating

Electron-neutrino dynamics in a supernova and constraints on the electron-neutrino magnetic moment 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 Electron-neutrino dynamics in a supernova and constraints on the electron-neutrino magnetic moment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Electron-neutrino dynamics in a supernova and constraints on the electron-neutrino magnetic moment will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-856106