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- W1621344225 abstract "Cooling of neutron stars (NSs) with the cores composed of neutrons, protons, and electrons is analyzed. The main cooling regulators are discussed: opening of direct Urca process in a NS central kernel; superfluidity of nucleons in NS interiors; surface layers of light (accreted) elements; strong surface magnetic fields. An emphasis is paid on the cooling scenario with strong $^1$S$_0$ pairing of protons and weak $^3$P$_2$ pairing of neutrons in the NS core, as well as strong $^1$S$_0$ pairing of neutrons in the NS crust. The theory predicts three types of isolated cooling middle-aged NSs with distinctly different properties: low-mass, slowly cooling NSs; medium-mass, moderately cooling NSs; massive, rapidly cooling NSs. The theory is compared with observations of isolated NSs -- pulsars and radio quiet NSs in supernova remnants. The constraints on physical properties of NSs which can be inferred from such a comparison are outlined." @default.
- W1621344225 created "2016-06-24" @default.
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- W1621344225 date "2002-04-13" @default.
- W1621344225 modified "2023-09-23" @default.
- W1621344225 title "Cooling of Superfluid Neutron Stars" @default.
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- W1621344225 hasPublicationYear "2002" @default.
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