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Space and Energy Distribution of Dark Matter

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dc.contributor.author Blitzner, Åsmund
dc.date.accessioned 2012-04-23T13:01:40Z
dc.date.available 2012-04-23T13:01:40Z
dc.date.issued 2011-11-17
dc.date.submitted 2011-11-17 en
dc.identifier.uri http://hdl.handle.net/1956/5764
dc.description.abstract I 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.extent 820715 bytes en
dc.format.mimetype application/pdf en
dc.language.iso eng en
dc.publisher The University of Bergen en
dc.title Space and Energy Distribution of Dark Matter en
dc.type Master thesis en
dc.type.degree Master i Fysikk en
dc.type.course PHYS399 en
dc.subject.nsi VDP::Mathematics and natural science: 400::Physics: 430 en
dc.subject.nsi VDP::Mathematics and natural science: 400::Physics: 430:aparticle physics: 431 en
dc.subject.archivecode Mastergrad en
dc.subject.nus 752199 en
dc.type.program MAMN-PHYS en


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