Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model - art. no. 038801

Authors
Panda, PK Sahu, R Das, C
Citation
Pk. Panda et al., Finite temperature neutron matter and rotating neutron stars in the quark meson coupling model - art. no. 038801, PHYS REV C, 6003(3), 1999, pp. 8801
Citations number
24
Categorie Soggetti
Physics
Journal title
PHYSICAL REVIEW C-NUCLEAR PHYSICS
ISSN journal
05562813 → ACNP
Volume
6003
Issue
3
Year of publication
1999
Database
ISI
SICI code
0556-2813(199909)6003:3<8801:FTNMAR>2.0.ZU;2-C
Abstract
A mean-field description of nonoverlaping nucleon bags bound by the self-co nsistent exchange of sigma, omega, and rho mesons is used to investigate th e properties of neutron matter at finite temperature. We use the equation o f state of zero temperature to study the rotating neutron star in the Komat su-Eriguchi-Hachisu method. The mass, radius, and angular velocity of the n eutron star are calculated and compared with the Walecka model. [S0556-2813 (99)04208-9].