Internal Constitution of Neutron and Strange Stars
| dc.creator | Glendenning, Norman K. | |
| dc.date | 1997-06-23 | |
| dc.date | 1997-06-24 | |
| dc.date.accessioned | 2026-07-07T09:02:12Z | |
| dc.date.available | 2026-07-07T09:02:12Z | |
| dc.description | In the first of these two lectures I will discuss the rich constitution of neutron stars as a consequence of the Pauli principle which is engaged by the dominance of gravity over the nuclear force. Three especially interesting phenomena are discussed in this contect--(1) a mechanism for the formation of low-mass black holes distinct in their mass-range from the black holes formed in the prompt collapse of an entire star, (2) a multilayered crystalline structure consisting of confined hadronic matter embedded in a background of deconfined quark matter (or vice versa) which occupies a many kilometer thick inner region, and (3) a clean and pronounced signal of the formation of quark matter in the interior of neutron stars. In the second lecture I will discuss the strange matter hypothesis, its viability as well as its consequences for compact stars and a new family of white dwarfs with dense nuclear matter central regions some orders of magnuitude greater than in ordinary white dwarfs. | |
| dc.description | 34 pages, 30 figures embedded, Latex with crckapb.sty. (October 1996, to appear in Proceedings ``The Many Faces of Neutron Stars'' Alpar et. al. eds. (Kluwer Academic Publishers, Dortrecht) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9706236 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9706236 | |
| dc.identifier | in ``The Many Faces of Neutron Stars'', Eds. Buccheri, van Paradjis and Alpar, Kluwer Academic Publishers, Dordrect/Boston/London, (1998) p 15 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/148546 | |
| dc.subject | Astrophysics | |
| dc.title | Internal Constitution of Neutron and Strange Stars | |
| dc.type | text |