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- W2020202274 endingPage "B1466" @default.
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- W2020202274 abstract "Calculations of the rates of the cooling reactions $n+nensuremath{rightarrow}n+p+{e}^{ensuremath{-}}+{ensuremath{nu}}_{e}$ and $n+{ensuremath{pi}}^{ensuremath{-}}ensuremath{rightarrow}n+{e}^{ensuremath{-}}+{ensuremath{nu}}_{e}$ are presented; the rates of the closely related muon-producing reactions and the four inverse processes are also given. Several different arguments are used to obtain estimates of the relavant matrix elements. The nucleons are assumed to form a normal Fermi fluid with a continuous excitation spectrum. The calculated cooling rates indicate that a neutron star containing quasifree pions would cool within a few days to a temperature so low that the star would be unobservable. The surface of a star that does not contain quasifree pions would cool to ${10}^{7}$ ifmmode^circelsetextdegreefi{}K in a few months and would reach 4ifmmodetimeselsetexttimesfi{}${10}^{6}$ ifmmode^circelsetextdegreefi{}K in about 100 years. The calculated cooling rates strongly indicate that the discrete x-ray sources located in the direction of the galactic center are not neutron stars." @default.
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- W2020202274 date "1965-12-06" @default.
- W2020202274 modified "2023-09-29" @default.
- W2020202274 title "Neutron Stars. II. Neutrino-Cooling and Observability" @default.
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- W2020202274 doi "https://doi.org/10.1103/physrev.140.b1452" @default.
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