Einstein Gravity from Conformal Gravity in 6D

Abstract

We extend Maldacena's argument, namely, obtaining Einstein gravity from Conformal Gravity, to six dimensional manifolds. The proof relies on a particular combination of conformal (and topological) invariants, which makes manifest the fact that 6D Conformal Gravity admits an Einstein sector. Then, by taking generalized Neumann boundary conditions, the Conformal Gravity action reduces to the renormalized Einstein-AdS action. These restrictions are implied by the vanishing of the traceless Ricci tensor, which is the defining property of any Einstein spacetime. The equivalence between Conformal and Einstein gravity renders trivial the Einstein solutions of 6D Critical Gravity at the bicritical point.

Energy of anti-de Sitter black holes in odd-dimensional Quadratic Curvature Gravity

“…A recent proposal to circumvent this limitation considers the proper embedding of Einstein-AdS theory in Conformal gravity[25].…”