The rigid Horowitz-Myers conjecture

Eric Woolgar

doi:10.1007/JHEP03(2017)104

paper

The rigid Horowitz-Myers conjecture

arXiv:1602.06197 · doi:10.1007/JHEP03(2017)104

Abstract

The "new positive energy conjecture" Horowitz and Myers (1999) probes a possible nonsupersymmetric AdS/CFT correspondence. We consider a version formulated for complete, asymptotically Poincaré-Einstein Riemannian metrics $(M, g)$ with bounded scalar curvature $R \geq - n (n - 1)$ . This version then asserts that any such $(M, g)$ must have mass not less than the mass $m_{0}$ of a metric $g_{0}$ induced on a time-symmetric slice of a certain AdS soliton spacetime. The conjecture remains unproved, having so far resisted standard techniques. Little is known other than that the conjecture is true for metrics which are sufficiently small perturbations of $g_{0}$ . We pose another test for the conjecture. We assume its validity and attempt to prove as a corollary the corresponding scalar curvature rigidity statement, that $g_{0}$ is the unique asymptotically Poincaré-Einstein metric with mass $m = m_{0}$ obeying $R \geq - n (n - 1)$ . Were a second such metric $g_{1}$ not isometric to $g_{0}$ to exist, it then may well admit perturbations of lower mass, contradicting the assumed validity of the conjecture. We find that the minimum mass metric must be static Einstein, so the problem is reduced to that of static uniqueness. When $n = 3$ the manifold is isometric to a time-symmetric slice of an AdS soliton spacetime, unless it has a non-compact horizon. En route we study the mass aspect, obtaining and generalizing known results. The mass aspect is (i) related to the holographic energy density, (ii) a weighted invariant under boundary conformal transformations when the bulk dimension is odd, and (iii) zero for negative Einstein manifolds with Einstein conformal boundary.

Statement and proof of Lemma 3.1 corrected, other minor changes

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Abstract

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