Linear Stability of the Equilibrium Points in the Photogravitational Elliptical Restricted Three Body Problem when the Bigger Primary is a Radiating Oblate Spheroid

dc.contributor.guideA K SINGH
dc.coverage.spatial
dc.creator.researcherARTI KUMARI
dc.date.accessioned2023-01-13T15:08:42Z
dc.date.available2023-01-13T15:08:42Z
dc.date.awarded
dc.date.completed2015
dc.date.registered
dc.description.abstractnewline
dc.description.note
dc.format.accompanyingmaterialDVD
dc.format.dimensions
dc.format.extent
dc.identifier.urihttp://hdl.handle.net/10603/445996
dc.languageEnglish
dc.publisher.institutionSCIENCE
dc.publisher.placeMuzaffarpur
dc.publisher.universityBabasaheb Bhimrao Ambedkar Bihar University
dc.relation
dc.rightsuniversity
dc.source.universityUniversity
dc.subject.keywordMathematics
dc.subject.keywordMathematics Interdisciplinary Applications
dc.subject.keywordPhysical Sciences
dc.titleLinear Stability of the Equilibrium Points in the Photogravitational Elliptical Restricted Three Body Problem when the Bigger Primary is a Radiating Oblate Spheroid
dc.title.alternative
dc.type.degreePh.D.

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