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dc.contributor.authorDeppmeier, Jacklyn
dc.date.accessioned2017-06-05T17:46:14Z
dc.date.available2017-06-05T17:46:14Z
dc.date.issued2017-04
dc.identifier.urihttps://scholarworks.montana.edu/xmlui/handle/1/12977
dc.description.abstractNeutron stars are extremely dense objects that are created during star deaths. They typically follow either a “standard” cooling process, or a faster “non-standard” cooling process. Non-standard cooling is caused by the presence of exotic particles such as pions, quarks, or hyperons in the core. This poster focuses on non-standard cooling using a quark core model. Cooling curves were created using a neutron star thermal evolution code modified to account for cores made of exotic particles. These models can be compared to previous models and experimental data to learn more about actual cooling behavior.en_US
dc.language.isoen_USen_US
dc.publisherMontana State Univeristyen_US
dc.titleNon-Standard Neutron Star Cooling Using a Quark Modelen_US
dc.typePresentationen_US
mus.citation.conferenceStudent Research Celebrationen_US
mus.citation.extentfirstpage1en_US
mus.citation.extentlastpage1en_US
mus.relation.collegeCollege of Letters & Scienceen_US
mus.relation.departmentPhysics.en_US
mus.relation.universityMontana State University - Bozemanen_US


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