Space Science Reviews

, Volume 74, Issue 3, pp 427–436

Urca processes in dense matter and neutron star cooling

  • Paweł Haensel
Article

DOI: 10.1007/BF00751429

Cite this article as:
Haensel, P. Space Sci Rev (1995) 74: 427. doi:10.1007/BF00751429

Abstract

Urca-processes were introduced into astrophysics by Gamow and Schoenberg in 1941. Neutrino cooling resulting from urca-processes plays an important role at the latest stages of evolution of massive stars. Recent work on neutrino emissivity of dense matter shows that neutrino cooling via urca-processes could determine the thermal evolution of young neutron stars and depends dramatically on the composition of the neutron star core. In particular, if a neutron star contains a central core in which the “direct urca-process” is operative, the cooling timescale shortens by many orders of magnitude.

Key words

dense matterneutron stars

Copyright information

© Kluwer Academic Publishers 1995

Authors and Affiliations

  • Paweł Haensel
    • 1
  1. 1.N. Copernicus Astronomical CenterPolish Academy of SciencesWarszawaPoland