Thermal radiation of neutron stars

Details Thermal radiation of neutron stars Thermal radiation of neutron stars

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987afz....26..251a&link_type=abstract

(Astrofizika, vol. 26, Mar.-Apr. 1987, p. 251-261) Astrophysics (ISSN 0571-7132), vol. 26, no. 2, Sept. 1987, p. 155-161. Transl

Astronomy and Astrophysics

Astrophysics

1

Neutron Stars, Stellar Evolution, Stellar Radiation, Thermal Radiation, Neutrinos, Photons, Pions, Stellar Luminosity, Surface Temperature

Scientific paper

Parameters of the thermal evolution of neutron stars are found whose hadronic matter contains a π-meson component. The surface temperature TR for typical neutron stars is shown to lie in the range of 105 ≤ TR ≤ 106. The cooling of neutron stars at TR > 106 is due to neutrino loss. For neutron stars of 103 - 106years lifetime photon luminosity lies within 1029 - 1033erg/s.

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