Time flat surfaces and the monotonicity of the spacetime Hawking mass
arXiv:1310.8638 · doi:10.1007/s00220-014-2162-2
Abstract
We identify a condition on spacelike 2-surfaces in a spacetime that is relevant to understanding the concept of mass in general relativity. We prove a formula for the variation of the spacetime Hawking mass under a uniformly area expanding flow and show that it is nonnegative for these so-called "time flat surfaces." Such flows generalize inverse mean curvature flow, which was used by Huisken and Ilmanen to prove the Riemannian Penrose inequality for one black hole. A flow of time flat surfaces may have connections to the problem in general relativity of bounding the mass of a spacetime from below by the quasi-local mass of a spacelike 2-surface contained therein.
23 pages; sign error fixed from previous version, statement of Theorem 1.1 changed accordingly
References in corpus (6)
- Quasilocal mass in general relativity
- Isometric embeddings into the Minkowski space and new quasi-local mass
- Generalized inverse mean curvature flows in spacetime
- Time flat surfaces and the monotonicity of the spacetime Hawking mass II
- Rigidity of time-flat surfaces in the Minkowski spacetime
- On curves with nonnegative torsion
Cited by in corpus (9)
- Geometrical inequalities bounding angular momentum and charges in General Relativity
- The asymptotic behaviour of the Hawking energy along null asymptotically flat hypersurfaces
- Time flat surfaces and the monotonicity of the spacetime Hawking mass II
- Four lectures on quasi-local mass
- Rigidity of time-flat surfaces in the Minkowski spacetime
- RG-2 flow, mass and entropy
- Uniformly Area Expanding Flows in Spacetimes
- Null Geometry and the Penrose Conjecture
- Recent Developments in the Penrose Conjecture