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- W1880453771 abstract "This review demonstrates that neutrino emission from dense hadronic component in neutron stars is subject of strong modifications due to collective effects in the matter. With the most important in-medium processes incorporated in the cooling code an overall agreement with available soft $X$ ray data can be easily achieved. With these findings so called standard and non-standard cooling scenarios are replaced by one general nuclear medium cooling scenario which relates slow and rapid neutron star coolings to the star masses (interior densities). In-medium effects take important part also at early hot stage of neutron star evolution decreasing the neutrino opacity for less massive and increasing for more massive neutron stars. A formalism for calculation of neutrino radiation from matter is presented that treats on equal footing one-nucleon and multiple-nucleon processes as well as reactions with resonance bosons and condensates." @default.
- W1880453771 created "2016-06-24" @default.
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- W1880453771 date "2000-09-06" @default.
- W1880453771 modified "2023-09-27" @default.
- W1880453771 title "Medium Effects in Neutrino Cooling of Neutron Stars" @default.
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