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Applications of the Gross-Pitaevskii equation to gravity

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dc.contributor Germani, Cristiano
dc.creator Cunillera García, Francesc
dc.date 2017-10-25T17:25:45Z
dc.date 2017-10-25T17:25:45Z
dc.date 2017-06
dc.date.accessioned 2024-12-16T10:25:45Z
dc.date.available 2024-12-16T10:25:45Z
dc.identifier http://hdl.handle.net/2445/117112
dc.identifier.uri http://fima-docencia.ub.edu:8080/xmlui/handle/123456789/19947
dc.description Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2017, Tutor: Cristiano Germani
dc.description In 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.
dc.format 5 p.
dc.format application/pdf
dc.language eng
dc.rights cc-by-nc-nd (c) Cunillera, 2017
dc.rights http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.rights info:eu-repo/semantics/openAccess
dc.source Treballs Finals de Grau (TFG) - Física
dc.subject Forats negres (Astronomia)
dc.subject Matèria condensada
dc.subject Treballs de fi de grau
dc.subject Black holes (Astronomy)
dc.subject Condensed matter
dc.subject Bachelor's theses
dc.title Applications of the Gross-Pitaevskii equation to gravity
dc.type info:eu-repo/semantics/bachelorThesis


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