On the growth of temperature within neutron stars

Details On the growth of temperature within neutron stars On the growth of temperature within neutron stars

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979afz....15..647u&link_type=abstract

(Astrofizika, vol. 15, Oct.-Dec. 1979, p. 647-655.) Astrophysics, vol. 15, no. 4, Apr. 1980, p. 429-433. Translation.

Astronomy and Astrophysics

Astrophysics

17

Neutron Stars, Stellar Structure, Stellar Temperature, Crystallization, Stellar Luminosity, Stellar Mass, Thermal Conductivity

Scientific paper

Analytic expressions are obtained that describe the variation of the temperature in the degenerate layers of the shell of a neutron star with electron heat conduction. The relativistic expression is used for the coefficient of thermal conductivity, and a possible crystallization of the ions is taken into account. For a neutron star with solar mass of 1 and radius of 10 km, the central temperature is calculated as a function of luminosity. It is shown that for sufficiently large luminosity the main temperature difference occurs across the layer of degenerate relativistic gas.

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