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- W2147769968 abstract "Neutron star cooling calculations are reported which employ improved physics in the calculation of the temperature drop through the atmosphere. The atmosphere microphysics is discussed briefly. The predicted neutron star surface temperatures, in the interesting interval 300 ≤ t (yr) ≤ 105, do not differ appreciably from the earlier results of Van Riper and Lamb (1981) for a non-magnetic star; for a magnetic star, the surface temperature is lower than in the previous work. Comparison with observational limits show that an exotic cooling mechanism such as neutrino emission from a pion-condensate or in the presence of percolating quarks, is not required, unless the existence of a neutron star in the Tycho or SN1006 supernova remnants is established." @default.
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- W2147769968 date "1983-01-01" @default.
- W2147769968 modified "2023-09-26" @default.
- W2147769968 title "Neutron Star Cooling: Effects of Envelope Physics" @default.
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- W2147769968 doi "https://doi.org/10.1007/978-94-009-7231-5_77" @default.
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