Neutron Stars—Cooling and Transport

Please use this identifier to cite or link to this item: http://hdl.handle.net/10045/51126
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Title: Neutron Stars—Cooling and Transport
Authors: Potekhin, Alexander Y. | Pons, José A. | Page, Dany
Research Group/s: Astrofísica Relativista
Center, Department or Service: Universidad de Alicante. Departamento de Física Aplicada
Keywords: Neutron stars | Magnetic fields | Dense matter | Thermal emission | Heat transport
Knowledge Area: Astronomía y Astrofísica
Issue Date: Oct-2015
Publisher: Springer Science+Business Media Dordrecht
Citation: Space Science Reviews. 2015, 191(1): 239-291. doi:10.1007/s11214-015-0180-9
Abstract: Observations of thermal radiation from neutron stars can potentially provide information about the states of supranuclear matter in the interiors of these stars with the aid of the theory of neutron-star thermal evolution. We review the basics of this theory for isolated neutron stars with strong magnetic fields, including most relevant thermodynamic and kinetic properties in the stellar core, crust, and blanketing envelopes.
Sponsor: The work of A.P. on the effects of strong magnetic fields on blanketing envelopes (Sect. 5.2 and Appendix B) has been supported by the Russian Science Foundation (grant 14-12-00316).
URI: http://hdl.handle.net/10045/51126
ISSN: 0038-6308 (Print) | 1572-9672 (Online)
DOI: 10.1007/s11214-015-0180-9
Language: eng
Type: info:eu-repo/semantics/article
Rights: © Springer Science+Business Media Dordrecht 2015. The final publication is available at Springer via http://dx.doi.org/10.1007/s11214-015-0180-9
Peer Review: si
Publisher version: http://dx.doi.org/10.1007/s11214-015-0180-9
Appears in Collections:INV - Astrofísica Relativista - Artículos de Revistas

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