Physics
Scientific paper
May 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phrvl..66.2425p&link_type=abstract
Physical Review Letters (ISSN 0031-9007), vol. 66, May 13, 1991, p. 2425-2428.
Physics
32
Heat Transfer, Stellar Envelopes, Stellar Physics, Stellar Temperature, Degenerate Matter, Relativistic Theory, Stellar Evolution, Stellar Models
Scientific paper
The cooling history of a strange star surrounded by a thin crust of ordinary matter is followed by solving analytically the general-relativistic equation of heat transfer across the crust. The surface temperature of the strange star is found to be lower than that of a neutron star (ordinary or with core condensates) of the same age. This provides a definite observational signature for these exotic objects, so far the first quantitative one to be proposed.
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