Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/117111
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dc.contributor.advisorWitek, Helvi-
dc.contributor.authorCreci, Gastón-
dc.date.accessioned2017-10-25T17:15:35Z-
dc.date.available2017-10-25T17:15:35Z-
dc.date.issued2017-06-
dc.identifier.urihttp://hdl.handle.net/2445/117111-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: Helvi Witekcat
dc.description.abstractWe solve the Klein-Gordon equation for an axion field in a Kerr background analytically for M [mu] << 1 and M [omega] << 1 for small spins via matching the near and far region solutions. This yields a hydrogen-like frequency spectrum and, if the superradiance condition is met, an instability. Moreover, we discuss some physically relevant elements of our system such as the potential associated to a black hole, the superradiance rate or the flux at the event horizon, comparing them with the numerical solution where our approximations are no longer valid.eng
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengeng
dc.rightscc-by-nc-nd (c) Creci, 2017-
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.classificationTreballs de fi de graucat
dc.subject.otherBlack holes (Astronomy)eng
dc.subject.otherBachelor's theseseng
dc.titleBlack holes and axionseng
dc.typeinfo:eu-repo/semantics/bachelorThesiseng
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesseng
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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