Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/598
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dc.contributor.advisorMinwalla, Shirazen_US
dc.contributor.authorDE, ANANDITAen_US
dc.date.accessioned2016-05-04T06:35:21Z
dc.date.available2016-05-04T06:35:21Z
dc.date.issued2016-01en_US
dc.identifier.citation1504.06613en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/598-
dc.description.abstractWe study the effective horizon dynamics of black holes in large number of dimensions($D$). To do this,we construct $SO(D-p-2)$ invariant solutions to Einstein's equations in large number of dimensions D in a power series expansion in $\frac{1}{D-3}$ holding $p$ fixed and finite. We find that the horizon dynamics of black holes in large D can be recast into a well-posed initial value problem of dynamics of a non gravitational co-dimension one membrane propagating in flat space. The dynamical degrees of freedom of this membrane are its shape function and a divergence free velocity field. We find the equation of motion governing the dynamics of this membrane upto first subleading order in $\frac{1}{D-3}$.en_US
dc.language.isoenen_US
dc.publisher1504.06613en_US
dc.subject2016
dc.subjectBlack Holes, Large Dimensionsen_US
dc.titleBlack Holes in Large Number of Dimensionsen_US
dc.typeThesisen_US
dc.type.degreeBS-MSen_US
dc.contributor.departmentDept. of Physicsen_US
dc.contributor.registration20111045en_US
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