The quark strange star in the enlarged Nambu-Jona-Lasinio model
| dc.creator | Manka, R. | |
| dc.creator | Bednarek, I. | |
| dc.creator | Przybyla, G. | |
| dc.date | 2002-01-03 | |
| dc.date | 2002-02-23 | |
| dc.date.accessioned | 2026-07-07T11:32:37Z | |
| dc.date.available | 2026-07-07T11:32:37Z | |
| dc.description | The strange quark star is investigated within the enlarged SU(3) Nambu-Jona-Lasinio (NJL). The stable quark star exists till maximal configutation with rho_m=3.1, 10^15, g/cm^3 with M_m=1.61, M_Sun and R_m=8.74, km is reached. Strange quarks appear for density above rho_c=9.84 g/cm^3 for the quark star with radius R_c=8.003 km and M_c=0.77, M_Sun. The comparison of a quark star properties obtained in the Quark Mean Field (QMF) approach to a neutron star model constructed within the Relativistic Mean Field (RMF) theory is presented. | |
| dc.description | 23 pages, iop latex2e + hyperref, 11 figures, to appear in NJP | |
| dc.identifier | https://arxiv.org/abs/nucl-th/0201003 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/0201003 | |
| dc.identifier | NewJ.Phys.4:14,2002 | |
| dc.identifier | doi:10.1088/1367-2630/4/1/314 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/197657 | |
| dc.subject | Nuclear Theory | |
| dc.title | The quark strange star in the enlarged Nambu-Jona-Lasinio model | |
| dc.type | text |