Classical and Quantum Gravity · 2017 · 14 citations · 11 references
Natural SciencesPhysicsGravitationGravityRelativityCurved SpacetimeGeneral RelativityAsymptotic FlatnessAsymptotically Flat SpacetimesCurvatureGaussian CurvatureMean CurvatureScalar CurvatureSchwarzschild GeometryUpper Bound Computation
Let $g$ be a metric on the $2$-sphere $\mathbb{S}^2$ with positive Gaussian curvature and $H$ be a positive constant. Under suitable conditions on $(g, H)$, we construct smooth, asymptotically flat $3$-manifolds $M$ with non-negative scalar curvature, with outer-minimizing boundary isometric to $(\mathbb{S}^2, g)$ and having mean curvature $H$, such that near infinity $M$ is isometric to a spatial Schwarzschild manifold whose mass $m$ can be made arbitrarily close to a constant multiple of the Hawking mass of $(\mathbb{S}^2,g,H)$. Moreover, this constant multiplicative factor depends only on $(g, H)$ and tends to $1$ as $H$ tends to $0$. The result provides a new upper bound of the Bartnik mass associated to such boundary data.
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Black holes in general relativity
S. W. Hawking · Communications in Mathematical Physics · 1972 · 1.6K citations
Natural Sciences, Physics, Cosmology +13
Coordinate Invariance and Energy Expressions in General Relativity
R. Arnowitt, S. Deser, Charles W. Misner · Physical Review · 1961 · 581 citations