Please use this identifier to cite or link to this item: https://hdl.handle.net/2445/201060
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dc.contributor.advisorBulashenko, Oleg-
dc.contributor.authorFernández Esteban, Juan-
dc.date.accessioned2023-07-24T07:16:09Z-
dc.date.available2023-07-24T07:16:09Z-
dc.date.issued2023-06-
dc.identifier.urihttps://hdl.handle.net/2445/201060-
dc.descriptionTreballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2023, Tutor: Oleg Bulashenkoca
dc.description.abstractGravitational waves open a new possibility in the detection of small dark matter halos. In this study we examine the gravitational lensing properties of the Navarro-Frenk-White (NFW) density profile, which is the most used model to describe cold dark matter halos. We also analyze the influence of the NFW halos on gravitational waves and, lastly, we study the effects of this interaction on the detection of the already mentioned waves. By exploring this effects, our objective is to understand better the interaction of gravitational waves and dark matter, two subjects shrouded in mistery.ca
dc.format.extent5 p.-
dc.format.mimetypeapplication/pdf-
dc.language.isoengca
dc.rightscc-by-nc-nd (c) Fernández, 2023-
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.sourceTreballs Finals de Grau (TFG) - Física-
dc.subject.classificationMatèria fosca (Astronomia)cat
dc.subject.classificationOnes gravitacionalscat
dc.subject.classificationTreballs de fi de graucat
dc.subject.otherDark matter (Astronomy)eng
dc.subject.otherGravitational waveseng
dc.subject.otherBachelor's theseseng
dc.titleProbing dark matter halos by gravitational waveseng
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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