Thermal conduction across neutron star crusts and cooling of young neutron stars

Details Thermal conduction across neutron star crusts and cooling of young neutron stars Thermal conduction across neutron star crusts and cooling of young neutron stars

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nupha.356..523r&link_type=abstract

Nuclear Physics A, Volume 356, Issue 2, p. 523-532.

Physics

Nuclear Physics

7

Scientific paper

We calculate thermal conduction times in the crust and core of a neutron star and find that for certain neutron star models the surface remains thermally isolated from the core at initial times. The surface temperature of a few hundred year old neutron star in these models can be insensitive to the presence of a pion-condensed core and might well be within the limits of observability of the HEAO satellite which can help to distinguish between different neutron star models.

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