Non-equilibrium neutrino emissivities and opacities of neutron star matter

Details Non-equilibrium neutrino emissivities and opacities of neutron star matter Non-equilibrium neutrino emissivities and opacities of neutron star matter

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...262..131h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 262, no. 1, p. 131-137.

Astronomy and Astrophysics

Astrophysics

32

Neutrinos, Neutron Stars, Nonequilibrium Conditions, Particle Emission, Stellar Mass, Density Distribution, Opacity, Stellar Composition

Scientific paper

The neutrino emissivity of neutron star matter out of the beta equilibrium is calculated. This condition can prevail in a neutron star matter undergoing rapid compression. The formulas for the neutrino emissivity from direct and modified beta processes are expressed in terms of the difference between the chemical potentials for the plasma composed of neutrons, protons, and electrons, delta mu = mu(n) - mu(p) - mu(e).

Affiliated with

Also associated with

No associations

Rating

Non-equilibrium neutrino emissivities and opacities of neutron star matter 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 Non-equilibrium neutrino emissivities and opacities of neutron star matter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-equilibrium neutrino emissivities and opacities of neutron star matter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1164365