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

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

2008-02-14

arxiv.org/abs/0802.1999v3

Astrophys.J.683:943-948,2008

Astronomy and Astrophysics

Astrophysics

Scientific paper

10.1086/589735

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 like 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 determine the maximum frequencies of rotation during the cooling.

Affiliated with

Also associated with

No associations

Rating

Proto-Neutron and Neutron Stars in a Chiral SU(3) Model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Proto-Neutron and Neutron Stars in a Chiral SU(3) Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Proto-Neutron and Neutron Stars in a Chiral SU(3) Model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-682509