The diffusion of weakly interacting particles from the proto-neutron star.

Details The diffusion of weakly interacting particles from the proto-neutron star. The diffusion of weakly interacting particles from the proto-neutron star.

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimb.105..835k&link_type=abstract

Nuovo Cimento B, Vol. 105, No. 8/9, p. 835 - 844

Physics

Neutron Stars: Elementary Particles, Neutron Stars: Diffusion

Scientific paper

The energy release of the proto-neutron star by the diffusion of the
neutrinos and the majoron-like particles is discussed. It is shown that
the majoron neutrino coupling is constrained from the observed neutrino
flux from SN 1987A. A possible way of extending the constraint is
briefly discussed.

Affiliated with

Also associated with

No associations

Rating

The diffusion of weakly interacting particles from the proto-neutron star. 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 The diffusion of weakly interacting particles from the proto-neutron star., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The diffusion of weakly interacting particles from the proto-neutron star. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1406010