Theory of cooling neutron stars versus observations

Yakovlev, D. G.; Gnedin, O. Y.; Kaminker, A. D.; Potekhin, A. Y.

doi:10.1063/1.2900259

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DOI

Theory of cooling neutron stars versus observations

Yakovlev, D. G.; Gnedin, O. Y.; Kaminker, A. D.; Potekhin, A. Y.
arXiv e-print [ PDF ]2008

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AbstractAbstract

[en] We review current state of neutron star cooling theory and discuss the prospects to constrain the equation of state, neutrino emission and superfluid properties of neutron star cores by comparing the cooling theory with observations of thermal radiation from isolated neutron stars

Primary Subject

CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS (S71)

Secondary Subject

PHYSICS OF ELEMENTARY PARTICLES AND FIELDS (S72)

Source

International conference on 40 years of pulsars: Millisecond pulsars, magnetars and more; Montreal (Canada); 12-17 Aug 2007; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA)

Record Type

Journal Article

Literature Type

Conference

Journal

AIP Conference Proceedings; ISSN 0094-243X;

; CODEN APCPCS; v. 983(1); p. 379-387

Country of publication

United States

Descriptors (DEI)

ASTROPHYSICS, COMPARATIVE EVALUATIONS, EQUATIONS OF STATE, NEUTRON STARS, NUCLEAR MATTER, PHOTON EMISSION, SUPERFLUIDITY, THERMAL RADIATION

Descriptors (DEC)

ELECTROMAGNETIC RADIATION, EMISSION, EQUATIONS, EVALUATION, MATTER, PHYSICS, RADIATIONS, STARS

LanguageLanguage

English

Reference NumberReference Number

40017375

INIS VolumeINIS Volume

INIS IssueINIS Issue

External URLExternal URL

http://dx.doi.org/10.1063/1.2900259

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