Nonstandard thermal evolution of neutron stars

Details Nonstandard thermal evolution of neutron stars Nonstandard thermal evolution of neutron stars

Sep 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...433..256u&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 433, no. 1, p. 256-264

Astronomy and Astrophysics

Astrophysics

35

Neutron Stars, Stellar Evolution, Stellar Models, Stellar Temperature, Superfluidity, Kaons, Mathematical Models, Neutrinos, Quarks

Scientific paper

A neutron star may cool much faster than through the 'standard' scenario. Here we calculate thermal evolution of neutron stars through various 'nonstandard' fast cooling scenarios, and the results are compared with the currently up-dated observational data. We discuss the possibility of distinguishing between the standard and various, different nonstandard scenarios, through the current and future X-ray satellite observations.

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