Susy transitions in compact objects

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dc.contributorJones, S. E.
dc.contributorHarms, B.
dc.contributorStancu, Ion
dc.contributorStern, Allen B.
dc.contributorHardee, P. E.
dc.contributorFrenkel, Alexander
dc.contributor.advisorClavelli, L.
dc.contributor.authorPerevalova, Irina A.
dc.contributor.otherUniversity of Alabama Tuscaloosa
dc.date.accessioned2017-02-28T22:30:48Z
dc.date.available2017-02-28T22:30:48Z
dc.date.issued2010
dc.descriptionElectronic Thesis or Dissertationen_US
dc.description.abstractFrom the very moment of discovery, gamma-ray bursts (GRB) became a very fascinating subject for study. Although this phenomena has been observed for four decades, the origin of such extraordinary events is yet to be discovered. In our research, we propose one possible explanation of the phenomena. We support our proposal with detailed theoretical calculations and computer simulations which give us confidence to consider the proposed model as consistent. The structure of the dissertation is the following: in the first chapter, after a brief introduction to the history of the GRB, we give a description of existing models of GRB origin, pointing out, however, the reasons why we cannot accept the models entirely. Then we give a review of the astronomical objects that will be important for our model. Finally in the end of the chapter we introduce our model. Chapter two is entirely theoretical. After a brief introduction of supersymmetry (SUSY) we provide the apparatus we used in later calculations. In chapter three we present the calculations for the fermion → s-fermion transition cross-sections for the Dirac sea and results of Monte Carlo simulations for these transitions. In chapter four we present different collective nuclear models and the results of numerical evaluations of the energy release during the SUSY transition. Energy balance for possible nuclear reactions is also provided in this chapter. Finally, we present our conclusions in chapter five.en_US
dc.format.extent71 p.
dc.format.mediumelectronic
dc.format.mimetypeapplication/pdf
dc.identifier.otheru0015_0000001_0000353
dc.identifier.otherPerevalova_alatus_0004D_10493
dc.identifier.urihttps://ir.ua.edu/handle/123456789/859
dc.languageEnglish
dc.language.isoen_US
dc.publisherUniversity of Alabama Libraries
dc.relation.hasversionborn digital
dc.relation.ispartofThe University of Alabama Electronic Theses and Dissertations
dc.relation.ispartofThe University of Alabama Libraries Digital Collections
dc.rightsAll rights reserved by the author unless otherwise indicated.en_US
dc.subjectPhysics, Elementary Particles and High Energy
dc.subjectPhysics, Theory
dc.titleSusy transitions in compact objectsen_US
dc.typethesis
dc.typetext
etdms.degree.departmentUniversity of Alabama. Department of Physics and Astronomy
etdms.degree.disciplinePhysics
etdms.degree.grantorThe University of Alabama
etdms.degree.leveldoctoral
etdms.degree.namePh.D.
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