Deconfinement Phase Transition Heating and Thermal Evolution of Neutron Stars - INSPIRE

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Deconfinement Phase Transition Heating and Thermal Evolution of Neutron Stars

Miao Kang
(
- Henan U. and
- Hua-Zhong Normal U.
)
,
Nana Pan
(
- Hua-Zhong Normal U.
)
,
Xiaodong Wang
(
- Henan U. and
- Hua-Zhong Normal U.
)

Nov, 2007

4 pages

Part of Astrophysics of compact objects. Proceedings, International Conference, Huangshan City, P.R. China, July 1-7, 2007, 203-205

Published in:

AIP Conf.Proc. 968 (2008) 1, 203-205

Contribution to:

International Conference on Astrophysics of Compact Objects, 203-205

Published: Jan 17, 2008

e-Print:

0711.0443 [astro-ph]

DOI:

10.1063/1.2840397

View in:

ADS Abstract Service

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Abstract: (AIP)

The deconfinement phase transition will lead to the release of latent heat during spins down of neutron stars if the transition is the first‐order one. We have investigated the thermal evolution of neutron stars undergoing such deconfinement phase transition. The results show that neutron stars may be heated to higher temperature. This feature could be particularly interesting for high temperature of low‐magnetic field millisecond pulsar at late stage.

neutron stars
phase transformations
pulsars
equations of state

References(24)

Figures(0)

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