Russo, J. G. (Jorge Guillermo)Neher Mestre, Narcís2023-07-272023-07-272023-02https://hdl.handle.net/2445/201287Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2016, Tutor: J. RussoIn 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).5 p.application/pdfengcc-by-nc-nd (c) Neher, 2023http://creativecommons.org/licenses/by-nc-nd/3.0/es/Forats negres (Astronomia)Simetria esfèricaTreballs de fi de grauBlack holes (Astronomy)Circular symmetryBachelor's thesesinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess