An Analytic Model of Radiating Spherical Gravitational Collapse
| dc.contributor.author | Grammenos, T. | en |
| dc.contributor.author | Kolassis, C. | en |
| dc.date.accessioned | 2015-11-24T18:33:03Z | |
| dc.date.available | 2015-11-24T18:33:03Z | |
| dc.identifier.issn | 0375-9601 | - |
| dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16681 | |
| dc.rights | Default Licence | - |
| dc.title | An Analytic Model of Radiating Spherical Gravitational Collapse | en |
| heal.abstract | The gravitational collapse of a radiating sphere consisting of a heat-conducting fluid with shear-free and radial motion is considered. In the exterior of the sphere we assume Vaidya's outgoing metric, while in the interior we have a neutrino flux described by a pure radiation term in the energy-momentum tensor. At first, a brief review including some new considerations of a similar, previously studied model, is given. Then, a new model is presented, in which the space-time interior to the collapsing sphere is conformally flat. | en |
| heal.access | campus | - |
| heal.fullTextAvailability | TRUE | - |
| heal.identifier.secondary | <Go to ISI>://A1992JN19900002 | - |
| heal.identifier.secondary | http://ac.els-cdn.com/037596019290796O/1-s2.0-037596019290796O-main.pdf?_tid=7fe61f6de5dd580996257e2c1d995cf1&acdnat=1334228593_488242b77f1f6a73abe511b3baff3673 | - |
| heal.journalName | Physics Letters A | en |
| heal.journalType | peer reviewed | - |
| heal.language | en | - |
| heal.publicationDate | 1992 | - |
| heal.recordProvider | Πανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιών | el |
| heal.type | journalArticle | - |
| heal.type.el | Άρθρο Περιοδικού | el |
| heal.type.en | Journal article | en |
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