On the consequence of neutrino trapping in gravitational collapse

Details On the consequence of neutrino trapping in gravitational collapse On the consequence of neutrino trapping in gravitational collapse

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...238..717g&link_type=abstract

Astrophysical Journal, Part 1, vol. 238, June 1, 1980, p. 717-721. Research supported by the U.S. Department of Energy and Mini

Astronomy and Astrophysics

Astrophysics

13

Gravitational Collapse, Neutrinos, Neutron Stars, Trapped Particles, Baryons, Entropy, Equations Of State, Stellar Models

Scientific paper

On the basis of very simple analytical considerations, it is shown how the strong trapping of neutrinos during stellar collapse has the effect of preventing nuclear dissociation. It is also shown how existing equations of state for neutrino-free matter (neutron star matter) can readily be extrapolated to arbitrarily neutrino-rich matter. Finally, models of neutron stars with trapped neutrinos are constructed, and their relevance for stellar collapse is discussed.

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