English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

We construct dynamical black hole solutions to Einstein Equations in presenceof matter in the large $D$ limit. The matter stress tensors that we considerare weak in the sense that they source asymptotic spacetimes with internalcurvatures of the order of $\mathcal{O}(D^0)$. Apart from this, we work with ageneric stress tensor demanding only that the stress tensor satisfies theconservation equations. The black hole solutions are obtained in terms of thedual non-gravitational picture of membranes propagating in spacetimesequivalent to the asymptotes of the black holes. We obtain the metric solutionsto the second sub-leading order in $1/D$. We also obtain the equationsgoverning the dual membranes up to the first sub-leading order in $1/D$.

Large $D$ Black Holes in an environment