Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/601
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dc.contributor.advisorBHATTACHARYAY, ARIJITen_US
dc.contributor.authorAGRAHAR, CHAITRAen_US
dc.date.accessioned2016-05-04T07:50:23Z
dc.date.available2016-05-04T07:50:23Z
dc.date.issued2016-05en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/601-
dc.description.abstractThe phenomenon of Hawking Radiation is explored in analogue gravity using Bose-Einstein Condensates. The process of spontaneous pair production that occurs at the event horizon is treated as a scattering problem, and the method of establishing Hawking Radiation using density correlations is reviewed. Based on the results obtained, the existing formalism is modified to incorporate the changes to the asymptotic modes due to the presence of the horizon.en_US
dc.description.sponsorshipINSPIRE Grant from DST, Government of India.en_US
dc.language.isoenen_US
dc.subject2016
dc.subjectHawking Radiationen_US
dc.subjectAnalogue Gravityen_US
dc.titleHawking Radiation in Analogue Gravityen_US
dc.typeThesisen_US
dc.type.degreeBS-MSen_US
dc.contributor.departmentDept. of Physicsen_US
dc.contributor.registration20111007en_US
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