This site uses cookies. By continuing to use this site you agree to our use of cookies. To find out more, see our Privacy and Cookies policy.

Proto-Neutron and Neutron Stars in a Chiral SU(3) Model

and

© 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation V. Dexheimer and S. Schramm 2008 ApJ 683 943 DOI 10.1086/589735

0004-637X/683/2/943

Abstract

A hadronic chiral SU(3) model is applied to neutron and proto-neutron stars, taking into account trapped neutrinos, finite temperature, and entropy. The transition to the chirally restored phase is studied, and global properties of the stars such as minimum and maximum masses and radii are calculated for different cases. In addition, the effects of rotation on neutron star masses are included, and the conservation of baryon number and angular momentum determines the maximum frequencies of rotation during the cooling.

Export citation and abstract BibTeX RIS

Please wait… references are loading.
10.1086/589735