Rearrangement of the Fermi Surface of Dense Neutron Matter and the Direct Urca Cooling of Neutron Stars

, , , and

Published 2000 April 7 © 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation D. N. Voskresensky et al 2000 ApJ 533 L127 DOI 10.1086/312607

1538-4357/533/2/L127

Abstract

It is proposed that a rearrangement of single-particle degrees of freedom may occur in a portion of the quantum-fluid interior of a neutron star. Such a rearrangement is associated with the pronounced softening of the spin-isospin collective mode which, under increasing density, leads to pion condensation. Arguments and estimates based on fundamental relations of many-body theory show that one realization of this phenomenon could produce very rapid cooling of the star via a direct nucleon Urca process displaying a T5 dependence on temperature.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/312607