Neutrino opacities and emissivities of importance in supernovae

Details Neutrino opacities and emissivities of importance in supernovae Neutrino opacities and emissivities of importance in supernovae

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975nyasa.262...65s&link_type=abstract

(AAS, American Physical Society, and New York Academy of Sciences, Texas Symposium on Relativistic Astrophysics, 7th, Dallas, Te

Astronomy and Astrophysics

Astrophysics

8

Emissivity, Gravitational Collapse, Neutrinos, Particle Emission, Scattering Cross Sections, Supernovae, Absorption Cross Sections, Coherent Scattering, Electron Capture, Electron Scattering, Mean Free Path, Nuclear Binding Energy, Radioactive Decay, Stellar Mass

Scientific paper

New calculations of neutrino emissivities and opacities under conditions of stellar collapse are made which take into account the presence of neutral currents and electron degeneracy effects. Estimates are made of the energy of a neutrino leaving the core of a collapsing object, and it is seen that the total energy of all neutrinos emitted can be greater than the binding energy of the material outside the core.

Affiliated with

Also associated with

No associations

Rating

Neutrino opacities and emissivities of importance in supernovae 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 opacities and emissivities of importance in supernovae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutrino opacities and emissivities of importance in supernovae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1746513