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Cooling of Neutron Stars: Accurate Treatment of Thermal Conduction

Published online by Cambridge University Press:  14 August 2015

N. Itoh ,
K. Nomoto ,
S. Tsuruta  and
T. Murai
N. Itoh
Affiliation:
Department of Physics, Sophia University, Tokyo 102, Japan
K. Nomoto
Affiliation:
NASA, Goddard Space Flight Center, Greenbelt, Maryland 20771, U.S.A.
S. Tsuruta
Affiliation:
Department of Physics, Montana State University, Bozeman, Montana 59717, U.S.A.
T. Murai
Affiliation:
Department of Physics, Nagoya University, Nagoya 464, Japan

Extract

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Most of the neutron star cooling calculations with the only exception of Malone's (1974) have assumed an isothermal stellar core. Here we report on a neutron star cooling calculation which makes full use of the stellar evolution code and the recent thermal conductivity calculations by Flowers and Itoh (1976, 1979).

Type
VII. Properties of Neutron Stars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 339 - 341
Copyright
Copyright © Reidel 1981 

References

Flowers, E. and Itoh, N.: 1976, Astrophys. J. 206, p. 218.CrossRefGoogle Scholar
Flowers, E. and Itoh, N.: 1979, Astrophys. J. 230, p. 847.Google Scholar
Malone, R.C.: 1974, , Cornell University, unpublished.Google Scholar
Pandharipande, V.R., Pines, D., and Smith, R.A.: 1976, Astrophys. J. 208, p. 550.Google Scholar