dc.contributor.advisor | Andersen, Jens Oluf | nb_NO |
dc.contributor.author | Berge, Eirik Samuel | nb_NO |
dc.date.accessioned | 2014-12-19T13:18:45Z | |
dc.date.available | 2014-12-19T13:18:45Z | |
dc.date.created | 2013-09-09 | nb_NO |
dc.date.issued | 2013 | nb_NO |
dc.identifier | 646886 | nb_NO |
dc.identifier | ntnudaim:6914 | nb_NO |
dc.identifier.uri | http://hdl.handle.net/11250/246997 | |
dc.description.abstract | In this thesis we will study the structure of quark stars using different models to mimic the interactions of quantum chromodynamics (QCD).The models we encounter is the MIT bag model and the two-and three-flavour linear sigma models with quark degrees of freedom. | nb_NO |
dc.language | eng | nb_NO |
dc.publisher | Institutt for fysikk | nb_NO |
dc.title | The Structure of Quark Stars | nb_NO |
dc.type | Master thesis | nb_NO |
dc.source.pagenumber | 111 | nb_NO |
dc.contributor.department | Norges teknisk-naturvitenskapelige universitet, Fakultet for naturvitenskap og teknologi, Institutt for fysikk | nb_NO |