Black Hole Shadows: Schwarzschild & Reissner-Nordström (anti-)dSitter

dc.contributor.advisor	Russo, J. G. (Jorge Guillermo)
dc.contributor.author	Neher Mestre, Narcís
dc.date.accessioned	2023-07-27T08:31:58Z
dc.date.available	2023-07-27T08:31:58Z
dc.date.issued	2023-02
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: J. Russo	ca
dc.description.abstract	In 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.extent	5 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/201287
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Neher, 2023
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.source	Treballs Finals de Grau (TFG) - Física
dc.subject.classification	Forats negres (Astronomia)	cat
dc.subject.classification	Simetria esfèrica	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Black holes (Astronomy)	eng
dc.subject.other	Circular symmetry	eng
dc.subject.other	Bachelor's theses	eng
dc.title	Black Hole Shadows: Schwarzschild & Reissner-Nordström (anti-)dSitter	eng
dc.type	info:eu-repo/semantics/bachelorThesis	ca

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