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dc.contributor.advisorEmparan García de Salazar, Roberto A.-
dc.contributor.authorNavarro Navarro, Núria-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Roberto Emparanca
dc.description.abstractBlack holes in four dimensions have to be topologically spherical, dynamically stable and uniquely characterized by their conserved charges. In higher dimensions, black holes are less constrained. Black hole solutions have been found with non-spherical horizon topology, and the same conserved charges can describe different types of black objects. This work presents a study of known exact black hole solutions in higher dimensions: the generalization of the Schwarzschild and Kerr metric (Schwarzschild-Tangherlini and Myers-Perry rotating in a single plane) and a brief introduction to black
dc.format.extent5 p.-
dc.rightscc-by-nc-nd (c) Navarro, 2020-
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationForats negres (Astronomia)cat
dc.subject.classificationVarietats topològiques de dimensió 4cat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherBlack holes (Astronomy)eng
dc.subject.otherFour-manifolds (Topology)eng
dc.subject.otherBachelor's theseseng
dc.titleBlack holes in higher dimensions [TFG]eng
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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