Please use this identifier to cite or link to this item:
https://hdl.handle.net/2440/17566
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Type: | Journal article |
Title: | Neutron stars and strange stars in the chiral SU(3) quark mean field model |
Author: | Wang, P. Lawley, S. Leinweber, D. Thomas, A. Williams, A. |
Citation: | Physical Review C: Nuclear Physics, 2005; 72(4):045801-1-045801-8 |
Publisher: | American Physical Soc |
Issue Date: | 2005 |
ISSN: | 0556-2813 1089-490X |
Statement of Responsibility: | P. Wang, S. Lawley, D. B. Leinweber, A. W. Thomas, and A. G. Williams |
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. |
Rights: | ©2005 American Physical Society. |
DOI: | 10.1103/PhysRevC.72.045801 |
Published version: | http://dx.doi.org/10.1103/physrevc.72.045801 |
Appears in Collections: | Aurora harvest 6 Special Research Centre for the Subatomic Structure of Matter publications |
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File | Description | Size | Format | |
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hdl_17566.pdf | Published version | 251.4 kB | Adobe PDF | View/Open |
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