Accretion ejection mechanism from advective accretion disc around rotating black holes

dc.contributor.guide	Das, Santabrata
dc.coverage.spatial	Physics
dc.creator.researcher	Aktar, Md Ramiz
dc.date.accessioned	2023-03-02T05:51:10Z
dc.date.available	2023-03-02T05:51:10Z
dc.date.awarded	2018
dc.date.completed	2018
dc.date.registered	2012
dc.description.abstract	In the first work we investigate the effect of spin on the mass outflow rates from a steady advective inviscid geometrically thin accretion flow around a rotating black hole For this purpose we adopt pseudo Kerr potentials to mimic the space time geometry around rotating black holes We calculate maximum outflow rates in terms of spin of the black holes Interestingly we observe a weak correlation between the spin and the maximum outflow rates from our model Finally we apply our accret
dc.description.note	Not Available
dc.format.accompanyingmaterial	None
dc.format.dimensions	Not Available
dc.format.extent	Not Available
dc.identifier.uri	http://hdl.handle.net/10603/465310
dc.language	English
dc.publisher.institution	DEPARTMENT OF PHYSICS
dc.publisher.place	Guwahati
dc.publisher.university	Indian Institute of Technology Guwahati
dc.relation	Not Available
dc.rights	self
dc.source.university	University
dc.subject.keyword	Physical Sciences
dc.subject.keyword	Physics
dc.subject.keyword	Physics Applied
dc.title	Accretion ejection mechanism from advective accretion disc around rotating black holes
dc.title.alternative	Not available
dc.type.degree	Ph.D.