Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/201287
Full metadata record
DC FieldValueLanguage
dc.contributor.advisorRusso, J. G. (Jorge Guillermo)-
dc.contributor.authorNeher Mestre, Narcís-
dc.date.accessioned2023-07-27T08:31:58Z-
dc.date.available2023-07-27T08:31:58Z-
dc.date.issued2023-02-
dc.identifier.urihttp://hdl.handle.net/2445/201287-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: J. Russoca
dc.description.abstractIn this work we discuss a precise derivation of shadows for spherically symmetric black holes. A brief overview of the historical Synge solution is also provided, along with a detailed explanation of the modern methodology that can be used with more complex metrics. The methodology will then be applied to some of the most significant black hole solutions. (Schwarzschild & Reissner-Nordström dSitter).ca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Neher, 2023-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationForats negres (Astronomia)cat
dc.subject.classificationSimetria esfèricacat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherBlack holes (Astronomy)eng
dc.subject.otherCircular symmetryeng
dc.subject.otherBachelor's theseseng
dc.titleBlack Hole Shadows: Schwarzschild & Reissner-Nordström (anti-)dSittereng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
Appears in Collections:Treballs Finals de Grau (TFG) - Física

Files in This Item:
File Description SizeFormat 
NEHER MESTRE NARCÍS_7934140.pdf326.04 kBAdobe PDFView/Open


This item is licensed under a Creative Commons License Creative Commons