Please use this identifier to cite or link to this item: http://hdl.handle.net/2445/188785
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dc.contributor.advisorCasalderrey Solana, Jorge-
dc.contributor.authorPonce de León Abad, Enric-
dc.date.accessioned2022-09-07T14:19:39Z-
dc.date.available2022-09-07T14:19:39Z-
dc.date.issued2022-06-
dc.identifier.urihttp://hdl.handle.net/2445/188785-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2022, Tutor: Jorge Casalderrey Solanaca
dc.description.abstractIn this work we analyse the dynamics of the bubbles responsible of cosmological phase transitions in the early Universe. To do so, the hydrodynamic profiles of a relativistic bubble are studied depending on its wall velocity, which characterises three different fluid velocity and enthalpy profiles: deflagrations, detonations and hybrids. The differences between the velocity profiles of these regimes may lead to different gravitational waves power spectra, which are potentially detectable in the foreseeable future and thus of great interest in cosmologyca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Ponce de León, 2022-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationCosmologiacat
dc.subject.classificationTransformacions de fase (Física estadística)cat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherCosmologyeng
dc.subject.otherPhase transformations (Statistical physics)eng
dc.subject.otherBachelor's theseseng
dc.titleBubble Dynamics in Cosmological Phase Transitionseng
dc.typeinfo:eu-repo/semantics/bachelorThesisca
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca
Appears in Collections:Treballs Finals de Grau (TFG) - Física

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