Neutron star evolution with internal heating

Details Neutron star evolution with internal heating Neutron star evolution with internal heating

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...346..808s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 346, Nov. 15, 1989, p. 808-822. Research supported by the John Simon Guggen

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Heating, Neutron Stars, Stellar Evolution, Stellar Interiors, Computational Astrophysics, Cooling, Pulsars, Stellar Luminosity, Stellar Rotation, Superfluidity

Scientific paper

The thermal evolution predicted by current models of the superfluid-crust interaction is noted to differ substantially from the thermal evolution predicted by models without internal heating as well as previous models of heating. Heating rates approaching the maximum predicted by current models enhance the photon luminosity of the star in the neutrino cooling era, and dramatically alter the thermal evolution in the photon cooling era. Standard cooling models are consistent with current pulsar temperature estimates and upper limits, except those for the Vela pulsar, which are lower than predicted.

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