Large $D$ Black Holes in an environment
Taniya Mandal, Arunabha Saha

TL;DR
This paper constructs large D black hole solutions in the presence of matter, using a membrane paradigm approach, and derives their metrics and membrane equations up to second and first sub-leading orders in 1/D.
Contribution
It provides a systematic construction of dynamical black holes with matter in the large D limit, extending previous vacuum solutions and deriving membrane equations at sub-leading orders.
Findings
Black hole solutions constructed up to second sub-leading order in 1/D.
Membrane equations derived up to first sub-leading order in 1/D.
Framework applicable to matter sources with weak stress tensors.
Abstract
We construct dynamical black hole solutions to Einstein Equations in presence of matter in the large limit. The matter stress tensors that we consider are weak in the sense that they source asymptotic spacetimes with internal curvatures of the order of . Apart from this, we work with a generic stress tensor demanding only that the stress tensor satisfies the conservation equations. The black hole solutions are obtained in terms of the dual non-gravitational picture of membranes propagating in spacetimes equivalent to the asymptotes of the black holes. We obtain the metric solutions to the second sub-leading order in . We also obtain the equations governing the dual membranes up to the first sub-leading order in .
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