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Strange Stars in the MIT Bag Model

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dc.contributor.advisor James Lattimer. en_US
dc.contributor.author Mielke, Charlotte en_US
dc.contributor.other Department of Physics en_US
dc.date.accessioned 2012-05-17T12:21:44Z
dc.date.accessioned 2015-04-24T14:48:25Z
dc.date.available 2012-05-17T12:21:44Z
dc.date.available 2015-04-24T14:48:25Z
dc.date.issued 2011-08-01 en_US
dc.identifier Mielke_grad.sunysb_0771M_10636.pdf en_US
dc.identifier.uri http://hdl.handle.net/1951/56074 en_US
dc.identifier.uri http://hdl.handle.net/11401/71657 en_US
dc.description.abstract We 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.sponsorship This work is sponsored by the Stony Brook University Graduate School in compliance with the requirements for completion of degree. en_US
dc.format Monograph en_US
dc.format.medium Electronic Resource en_US
dc.language.iso en_US en_US
dc.publisher The Graduate School, Stony Brook University: Stony Brook, NY. en_US
dc.subject.lcsh Physics -- Astrophysics en_US
dc.subject.other MIT Bag Model, Quark Stars, Strange Stars en_US
dc.title Strange Stars in the MIT Bag Model en_US
dc.type Thesis en_US
dc.mimetype Application/PDF en_US
dc.contributor.committeemember Alan Calder en_US
dc.contributor.committeemember Maria Victoria Fernandez-Serra. en_US

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