On a mass functional for initial data in 4+1 dimensional spacetime
arXiv:1411.0609 · doi:10.1103/PhysRevD.90.124078
Abstract
We consider a broad class of asymptotically flat, maximal initial data sets satisfying the vacuum constraint equations, admitting two commuting rotational symmetries. We construct a mass functional for `' symmetric data which evaluates to the ADM mass. We then show that -invariant solutions of the vacuum Einstein equations are critical points of this functional amongst this class of data. We demonstrate positivity of this functional for a class of rod structures which include the Myers-Perry initial data. The construction is a natural extension of Dain's mass functional to , although several new features arise.
V2: 31 pages-Section 2.2 revised and lengthened (differs from published version); minor typos corrected
References in corpus (22)
- Stationary and Axisymmetric Solutions of Higher-Dimensional General Relativity
- Black Rings
- Uniqueness theorem for 5-dimensional black holes with two axial Killing fields
- Stability of Black Holes and Black Branes
- Einstein Constraints on Asymptotically Euclidean Manifolds
- Area - Angular momentum inequality for axisymmetric black holes
- Black hole Area-Angular momentum inequality in non-vacuum spacetimes
- Rod-structure classification of gravitational instantons with U(1)xU(1) isometry
- Black hole instabilities and local Penrose inequalities
- Geometric inequalities for axially symmetric black holes
- Black hole non-uniqueness via spacetime topology in five dimensions
- On the uniqueness of extremal vacuum black holes
- Mass, angular-momentum, and charge inequalities for axisymmetric initial data
- The Positive Mass and Isoperimetric Inequalities for Axisymmetric Black Holes in four and five dimensions
- Proof of the (local) angular momemtum-mass inequality for axisymmetric black holes
- The first law of soliton and black hole mechanics in five dimensions
- A variational principle for stationary, axisymmetric solutions of Einstein's equations
- The inequality between mass and angular momentum for axially symmetric black holes
- Instabilities of extremal rotating black holes in higher dimensions
- Horizon area-angular momentum inequality in higher dimensional spacetimes
- On the linear stability of the extreme Kerr black hole under axially symmetric perturbations
- Notes on maximal slices of five-dimensional black holes