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dc.contributor.authorMielke, Charlotteen_US
dc.contributor.otherDepartment of Physicsen_US
dc.date.accessioned2012-05-17T12:21:44Z
dc.date.available2012-05-17T12:21:44Z
dc.date.issued1-Aug-11en_US
dc.date.submittedAug-11en_US
dc.identifierMielke_grad.sunysb_0771M_10636.pdfen_US
dc.identifier.urihttp://hdl.handle.net/1951/56074
dc.description.abstractWe study strange stars under the assumption of the strange matter hypothesis, using an MIT bag model to describe strange matter. We find that a 1.97 solar masses star (as recently measured) is generally possible in the context of the bag model, although it places restrictions on the bag model's parameters. Furthermore, limits for the central pressure and energy density are obtained.en_US
dc.description.sponsorshipStony Brook University Libraries. SBU Graduate School in Department of Physics. Lawrence Martin (Dean of Graduate School).en_US
dc.formatElectronic Resourceen_US
dc.language.isoen_USen_US
dc.publisherThe Graduate School, Stony Brook University: Stony Brook, NY.en_US
dc.subject.lcshPhysics -- Astrophysicsen_US
dc.subject.otherMIT Bag Model, Quark Stars, Strange Starsen_US
dc.titleStrange Stars in the MIT Bag Modelen_US
dc.typeThesisen_US
dc.description.advisorAdvisor(s): James Lattimer. Committee Member(s): Alan Calder; Maria Victoria Fernandez-Serra.en_US
dc.mimetypeApplication/PDFen_US


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