Massive neutrinos in strong gravitational fields

Details Massive neutrinos in strong gravitational fields Massive neutrinos in strong gravitational fields

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ncimb..65...79d&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 65 B, Sept. 11, 1981, p. 79-88. Research supported by the Scuola Internazionale Superiore di Stu

Astronomy and Astrophysics

Astronomy

Black Holes (Astronomy), Equations Of State, Gravitational Fields, Neutrinos, Neutron Stars, Trapped Particles, Electron Density (Concentration), Gravitational Collapse, Particle Mass, Proton Density (Concentration), Stellar Interiors, Stellar Mass

Scientific paper

The gravitational field interior to condensed objects is able to trap neutrinos. If this phenomenon is consistent, it is argued that the trapped neutrinos can affect significantly the star interior; here we investigate this possibility in the case of massive neutrinos and find that they should contribute to the equation of state at the center of the star in the extreme phase of collapse before a black hole is formed.

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