Current Status of Neutron Star Thermal Evolution Theories

Details Current Status of Neutron Star Thermal Evolution Theories Current Status of Neutron Star Thermal Evolution Theories

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..362..111t&link_type=abstract

The Seventh Pacific Rim Conference on Stellar Astrophysics, ASP Conference Series, Vol. 362, Proceedings of the conference held

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Recent years have seen some significant progress in theoretical studies of the physics of dense matter. Combined with the observational data now available from the successful launch of Chandra and XMM/Newton X-ray space missions as well as various lower-energy band observations, these developments now offer the hope for distinguishing among various competing neutron star thermal evolution models. Consequently, we can now hope to determine various important properties, such as the composition, superfluidity, the equation of state and stellar radius of these stars.

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