Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/1615
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dc.contributor.authorPandya, Dhruv.-
dc.contributor.authorBagla, J.S.-
dc.contributor.authorSingh, Kulinder Pal-
dc.date.accessioned2021-12-09T17:38:52Z-
dc.date.available2021-12-09T17:38:52Z-
dc.date.issued2021-07-28-
dc.identifier.urihttp://hdl.handle.net/123456789/1615-
dc.description.abstractThe present thesis work is motivated by the detection of MCVs in 2018.Radiation detected from them was circularly polarized, had narrowbandwidth, had very high brightness temperature. Such radiation profile can be explained using the model of cyclotron maser instability. Present thesis work is an attempt to understand cyclotron maser in the context of MCVs. A novel Approach to obtain angular and spectral profile of the radiation from an accelerated particle using Maxwell’s equations on curved space time is discussed. Vlasov equation and a variant of H theorem for collisionless plasma are independently derived.en_US
dc.language.isoen_USen_US
dc.publisherIISERMen_US
dc.subjectCyclotronen_US
dc.subjectMaseren_US
dc.subjectInstabilityen_US
dc.titleTo Cyclotron Maser Instabilityen_US
dc.typeThesisen_US
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