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Space Science Reviews

, Volume 74, Issue 3–4, pp 427–436 | Cite as

Urca processes in dense matter and neutron star cooling

  • Paweł Haensel
Article

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 matter neutron stars 

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Copyright information

© Kluwer Academic Publishers 1995

Authors and Affiliations

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

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