Please use this identifier to cite or link to this item: https://olympias.lib.uoi.gr/jspui/handle/123456789/15850
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dc.contributor.authorSimon, Creeken
dc.contributor.authorRuth, Gregoryen
dc.contributor.authorPanagiota, Kantien
dc.contributor.authorBina, Mistryen
dc.date.accessioned2015-11-24T17:58:57Z-
dc.date.available2015-11-24T17:58:57Z-
dc.identifier.issn0264-9381-
dc.identifier.urihttps://olympias.lib.uoi.gr/jspui/handle/123456789/15850-
dc.rightsDefault Licence-
dc.titleBraneworld stars and black holesen
heal.typejournalArticle-
heal.type.enJournal articleen
heal.type.elΆρθρο Περιοδικούel
heal.identifier.secondaryhttp://stacks.iop.org/0264-9381/23/i=23/a=004-
heal.accesscampus-
heal.recordProviderΠανεπιστήμιο Ιωαννίνων. Σχολή Επιστημών και Τεχνολογιών. Τμήμα Βιολογικών Εφαρμογών και Τεχνολογιώνel
heal.publicationDate2006-
heal.abstractWe 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.journalNameClassical and Quantum Gravityen
heal.journalTypepeer reviewed-
heal.fullTextAvailabilityTRUE-
Appears in Collections:Άρθρα σε επιστημονικά περιοδικά ( Ανοικτά) - ΦΥΣ

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