Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model

Details Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phrvc..60c8801p&link_type=abstract

Physical Review C (Nuclear Physics), Volume 60, Issue 3, September 1999, id. 038801

Other

12

Nuclear Matter, Bag Model, Other Nonperturbative Calculations, Nuclear Matter Aspects Of Neutron Stars

Scientific paper

A mean-field description of nonoverlaping nucleon bags bound by the self-consistent exchange of σ, ω, and ρ mesons is used to investigate the properties of neutron matter at finite temperature. We use the equation of state of zero temperature to study the rotating neutron star in the Komatsu-Eriguchi-Hachisu method. The mass, radius, and angular velocity of the neutron star are calculated and compared with the Walecka model.

Affiliated with

Also associated with

No associations

Rating

Finite temperature neutron matter and rotating neutron stars in the quark meson coupling 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 Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-989114