Braneworld stars and black holes
dc.contributor.author | Simon, Creek | en |
dc.contributor.author | Ruth, Gregory | en |
dc.contributor.author | Panagiota, Kanti | en |
dc.contributor.author | Bina, Mistry | en |
dc.date.accessioned | 2015-11-24T18:32:29Z | |
dc.date.available | 2015-11-24T18:32:29Z | |
dc.identifier.issn | 0264-9381 | - |
dc.identifier.uri | https://olympias.lib.uoi.gr/jspui/handle/123456789/16576 | |
dc.rights | Default Licence | - |
dc.title | Braneworld stars and black holes | en |
heal.abstract | We look for spherically symmetric star or black hole solutions on a Randall Sundrum brane from the perspective of the bulk. We take a known bulk solution, and analyse possible braneworld trajectories within it that correspond, from the braneworld point of view, to solutions of the brane Tolman Oppenheimer Volkoff equations. Our solutions are therefore embedded consistently into a full bulk solution. We find the full set of static gravitating matter sources on a brane in a range of bulk spacetimes, analysing which can correspond to physically sensible sources. Finally, we look at time-dependent trajectories in a Schwarzschild anti-de Sitter spacetime as possible descriptions of time-dependent braneworld black holes, highlighting some of the general features one might expect, as well as some of the difficulties involved in getting a full solution to the question. | en |
heal.access | campus | - |
heal.fullTextAvailability | TRUE | - |
heal.identifier.secondary | http://stacks.iop.org/0264-9381/23/i=23/a=004 | - |
heal.journalName | Classical and Quantum Gravity | en |
heal.journalType | peer reviewed | - |
heal.publicationDate | 2006 | - |
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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