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• W2038814008 endingPage "130" @default.
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• W2038814008 abstract "After a brief introduction we present a progress report on the recent works carried out during the last ten years or so, on the thermal evolution of neutron stars and related problems. The effects of various improvements applied in recent years are discussed. Among these the most important may be the effects of magnetic fields and stellar atmospheres. When the problem is treated realistically with the two-dimensional method a magnetic neutron star appears to be kept warmer for a longer period, due to the tangential heat flow from the more insulated equatorial regions to the polar areas where heat escapes more efficiently. Possibly serious implications of this finding in relation to the interpretation of the observational data are discussed. The composition of the stellar atmosphere may be an important factor when we are to correctly interpret the observed temperature data. The current theoretical and observational considerations may support a ‘best buy model’, where some neutron stars with mass close to 1.4M⊙ possess a central core in which a ‘non-standard’ accelerating cooling mechanism, under the influence of significant suppression due to the presence of superfluid particles, is in operation. On the other hand, some less massive stars can still cool with the standard scenario. Some other interesting problems to be reviewed include: the most recent work on various ‘non-standard’ cooling scenarios; the pulsed radiation to be expected from magnetized neutron stars due to the anisotropic nature of conductivity and photon fluxes; the possible importance of the effects of various heating mechanisms and circumstellar electron positron pairs; the detectability of infant neutron stars in very young supernova remnants; and some applications to particle physics and cosmology. The topics to be covered are not meant to be complete, but the emphasis is placed on potentially interesting problems in relation to the recent and future observations of pulsars." @default.
• W2038814008 created "2016-06-24" @default.
• W2038814008 creator A5064735223 @default.
• W2038814008 date "1998-01-01" @default.
• W2038814008 modified "2023-10-18" @default.
• W2038814008 title "Thermal properties and detectability of neutron stars. II. Thermal evolution of rotation-powered neutron stars" @default.
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