Theory of cooling neutron stars versus observations

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dc.creatorYakovlev, D. G.
dc.creatorGnedin, O. Y.
dc.creatorKaminker, A. D.
dc.creatorPotekhin, A. Y.
dc.date2007-10-10
dc.date2007-12-12
dc.date.accessioned2026-07-07T11:12:07Z
dc.date.available2026-07-07T11:12:07Z
dc.descriptionWe 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.
dc.description9 pages, 4 figures, 3 tables, to appear in the proceedings of "40 Years of Pulsars" held in Montreal, Canada, August 12-17, 2007, eds. C. Bassa, Z. Wang, A. Cumming, V. Kaspi, AIP, in press (v.2 - minor bibliography corrections)
dc.identifierhttps://arxiv.org/abs/0710.2047
dc.identifierhttp://arxiv.org/abs/0710.2047
dc.identifierAIPConf.Proc.983:379-387,2008
dc.identifierdoi:10.1063/1.2900259
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191275
dc.subjectAstrophysics
dc.titleTheory of cooling neutron stars versus observations
dc.typetext

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