Gravitational waves from a neutron star merger

dc.contributor.advisor	Centelles Aixalà, Mario
dc.contributor.author	Bergonyó Forcades, Roger
dc.date.accessioned	2020-09-30T14:23:00Z
dc.date.available	2020-09-30T14:23:00Z
dc.date.issued	2020-06
dc.description	Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2020, Tutor: Mario Centelles Aixalà	ca
dc.description.abstract	In this work we present the equations that describe the structure of neutron stars, as well as different models that describe the properties of the neutron star matter, using Skyrme nuclear interactions. From the data obtained in the gravitational waves detected in recent years we determine which models are still valid to describe the neutron star matter and which are not.	ca
dc.format.extent	5 p.
dc.format.mimetype	application/pdf
dc.identifier.uri	https://hdl.handle.net/2445/170971
dc.language.iso	eng	ca
dc.rights	cc-by-nc-nd (c) Bergonyó, 2020
dc.rights.accessRights	info:eu-repo/semantics/openAccess	ca
dc.rights.uri	http://creativecommons.org/licenses/by-nc-nd/3.0/es/	*
dc.source	Treballs Finals de Grau (TFG) - Física
dc.subject.classification	Ones gravitacionals	cat
dc.subject.classification	Estels de neutrons	cat
dc.subject.classification	Treballs de fi de grau	cat
dc.subject.other	Gravitational waves	eng
dc.subject.other	Neutron stars	eng
dc.subject.other	Bachelor's theses	eng
dc.title	Gravitational waves from a neutron star merger	eng
dc.type	info:eu-repo/semantics/bachelorThesis	ca

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