Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/3853
Full metadata record
DC FieldValueLanguage
dc.contributor.authorPandya, Dhruv.-
dc.date.accessioned2021-09-13T10:52:24Z-
dc.date.available2021-09-13T10:52:24Z-
dc.date.issued2021-07-28-
dc.identifier.urihttp://hdl.handle.net/123456789/3853-
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.isoenen_US
dc.publisherIISERMen_US
dc.subjectCyclotronen_US
dc.subjectMaseren_US
dc.subjectInstabilityen_US
dc.titleTo Cyclotron Maser Instabilityen_US
dc.typeThesisen_US
dc.guideBagla, J.S.-
dc.guideSingh, Kulinder Pal-
Appears in Collections:MS-16

Files in This Item:
File Description SizeFormat 
It is under embargo period.docx11.62 kBMicrosoft Word XMLView/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.