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dc.contributor.authorBlitzner, Åsmundeng
dc.date.accessioned2012-04-23T13:01:40Z
dc.date.available2012-04-23T13:01:40Z
dc.date.issued2011-11-17eng
dc.date.submitted2011-11-17eng
dc.identifier.urihttp://hdl.handle.net/1956/5764
dc.description.abstractI start by an introduction to the notion of, and motivation for, Dark Matter, as well as a short motivation for supersymmetry, the theoretical framework usually examined when looking for places that dark matter may hide. After assuming a gravitino undergoing g → νγ decay, as a matter of convenience, there follows an exposition and use of the necessary tools to calculate the flux one might expect from galactic and extragalactic sources under such circumstances. The galactic model choice is given only a cursory glance, in anticipation of its ultimately minor importance to my main goal. That is, to determine if the decay of gravitinos over cosmological timescales is something that could influence our signal for reasonable values of the mean life.en
dc.format.extent820715 byteseng
dc.format.mimetypeapplication/pdfeng
dc.language.isoengeng
dc.publisherThe University of Bergeneng
dc.titleSpace and Energy Distribution of Dark Mattereng
dc.typeMaster thesiseng
dc.type.degreeMaster i Fysikknob
dc.type.coursePHYS399eng
dc.subject.nsiVDP::Mathematics and natural science: 400::Physics: 430eng
dc.subject.nsiVDP::Mathematics and natural science: 400::Physics: 430:aparticle physics: 431eng
dc.subject.archivecodeMastergradeng
dc.subject.nus752199eng
dc.type.programMAMN-PHYSeng


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