Neutron stars and strange stars in the chiral SU(3) quark mean field model
Files
(Published version)
Date
2005
Authors
Wang, P.
Lawley, S.
Leinweber, D.
Thomas, A.
Williams, A.
Editors
Advisors
Journal Title
Journal ISSN
Volume Title
Type:
Journal article
Citation
Physical Review C: Nuclear Physics, 2005; 72(4):045801-1-045801-8
Statement of Responsibility
P. Wang, S. Lawley, D. B. Leinweber, A. W. Thomas, and A. G. Williams
Conference Name
Abstract
We investigate the equations of state for pure neutron matter and strange hadronic matter in $\beta$-equilibrium, including $\Lambda$, $\Sigma$ and $\Xi$ hyperons. The masses and radii of pure neutron stars and strange hadronic stars are obtained. For a pure neutron star, the maximum mass is about $1.8 M_{\mathrm{sun}}$, while for a strange hadronic star, the maximum mass is around $1.45 M_{\mathrm{sun}}$. The typical radii of pure neutron stars and strange hadronic stars are about 11.0-12.3 km and 10.7-11.7 km, respectively.
School/Discipline
Dissertation Note
Provenance
Description
Access Status
Rights
©2005 American Physical Society.