Field theoretical model for nuclear and neutron matter. V - Slowly rotating warm cores in neutron stars

Details Field theoretical model for nuclear and neutron matter. V - Slowly rotating warm cores in neutron stars Field theoretical model for nuclear and neutron matter. V - Slowly rotating warm cores in neutron stars

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...395..612r&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 395, no. 2, Aug. 20, 1992, p. 612-621. Research supported by CICYT and Fulb

Physics

8

Equations Of State, Gravitation Theory, Neutron Stars, Stellar Interiors, Stellar Rotation, Baryons, Field Theory (Physics), Light Curve, Pulsars, Stellar Mass

Scientific paper

We have studied the macroscopic properties of general relativistic
slowly rotating warm neutron stars obeying the hot extension of an
equation of state derived recently in the realm of a field theoretical
model. Our results could be of interest in simulations of the early
Kelvin epoch of a rotating protoneutron star.

Affiliated with

Also associated with

No associations

Rating

Field theoretical model for nuclear and neutron matter. V - Slowly rotating warm cores in neutron stars 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 Field theoretical model for nuclear and neutron matter. V - Slowly rotating warm cores in neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Field theoretical model for nuclear and neutron matter. V - Slowly rotating warm cores in neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1165881