Effects of rotochemical heating on the thermal evolution of superfluid neutron stars

Details Effects of rotochemical heating on the thermal evolution of superfluid neutron stars Effects of rotochemical heating on the thermal evolution of superfluid neutron stars

2010-05-25

arxiv.org/abs/1005.4473v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

7 pages, 2 figures. To appear in Proceedings for "Compact stars in the QCD phase diagram II (CSQCD II), May 20-24, 2009, KIAA

Scientific paper

The authors take the rotochemical heating effect into account, which may make
the cooling scenario different. Their model is consistent with the observation
data.

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