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dc.contributor.advisorWang, Qiu-dongen_US
dc.contributor.authorPunosevac, Predrag
dc.creatorPunosevac, Predragen_US
dc.date.accessioned2011-12-05T22:31:04Z
dc.date.available2011-12-05T22:31:04Z
dc.date.issued2007en_US
dc.identifier.urihttp://hdl.handle.net/10150/194380
dc.description.abstractThe aim of this study is to construct coordinate transforms that regularize the singularities of simultaneous binary collisions in the Newtonian gravitational systems. Explicit regularization transforms are introduced for a pair of decoupled Kepler problems, a restricted collinear four-body problem, and the collinear four-body problem. This is the first time such transforms are produced for collisions involving more than one colliding pairs in the study of the Newtonian gravitational systems.
dc.language.isoENen_US
dc.publisherThe University of Arizona.en_US
dc.rightsCopyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author.en_US
dc.subjectMathematicsen_US
dc.titleRegularization of Simultaneous Binary Collisions in Some Gravitational Systemsen_US
dc.typetexten_US
dc.typeElectronic Dissertationen_US
dc.contributor.chairWang, Qiu-dongen_US
dc.identifier.oclc659747131en_US
thesis.degree.grantorUniversity of Arizonaen_US
thesis.degree.leveldoctoralen_US
dc.contributor.committeememberErcolani, Nicholasen_US
dc.contributor.committeememberCushing, Jimen_US
dc.contributor.committeememberHu, Yien_US
dc.identifier.proquest2051en_US
thesis.degree.disciplineMathematicsen_US
thesis.degree.disciplineGraduate Collegeen_US
thesis.degree.namePhDen_US
refterms.dateFOA2018-04-25T19:40:08Z
html.description.abstractThe aim of this study is to construct coordinate transforms that regularize the singularities of simultaneous binary collisions in the Newtonian gravitational systems. Explicit regularization transforms are introduced for a pair of decoupled Kepler problems, a restricted collinear four-body problem, and the collinear four-body problem. This is the first time such transforms are produced for collisions involving more than one colliding pairs in the study of the Newtonian gravitational systems.


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