Black holes in presence of cosmological constant: Second order in 1/D

Understand

We have extended the results of arXiv:1704.06076 upto second subleading order in an expansion around large dimension D.

• Unlike the previous case, there are non-trivial metric corrections at this order.
• Due to our `background-covariant' formalism, the dependence on Ricci and the Riemann curvature tensor of the background is manifest here.
• The gravity system is dual to a dynamical membrane coupled with a velocity field.