Germani, CristianoCunillera García, Francesc2017-10-252017-10-252017-06https://hdl.handle.net/2445/117112Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: Cristiano GermaniIn this paper the main characteristics of the interior solution of a static black hole as a Bose-Einstein condensate of gravitons are explored. We find that, even up to the boundary of the black hole, quantum corrections cannot be ignored which in turn leads to the conclusion that, in this framework, not even in the classical limit the interior of the black hole is described adequately by General Relativity. Furthermore, a non-singular interior solution is found.5 p.application/pdfengcc-by-nc-nd (c) Cunillera, 2017http://creativecommons.org/licenses/by-nc-nd/3.0/es/Forats negres (Astronomia)Matèria condensadaTreballs de fi de grauBlack holes (Astronomy)Condensed matterBachelor's thesesApplications of the Gross-Pitaevskii equation to gravityinfo:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/openAccess