The cooling of white dwarfs with allowance for nonequilibrium beta processes

Details The cooling of white dwarfs with allowance for nonequilibrium beta processes The cooling of white dwarfs with allowance for nonequilibrium beta processes

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13.1014b&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Nov. 1987, p. 1014-1018. In Russian.

Astronomy and Astrophysics

Astronomy

Cool Stars, Nonequilibrium Conditions, Stellar Evolution, White Dwarf Stars, Chromium, Heating, Neutrons, Stellar Cores

Scientific paper

The nonequilibrium heating of a white dwarf during two-step
neutronization and the formation of a small but finite core of the new
phase is investigated. It is shown that this nonequilibrium heating is
the main source of energy when the Coulomb crystal becomes degenerate.

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