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On the existence of rigid spheres in four-dimensional spacetime manifolds

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TLDR
In this paper, the authors considered geometric properties of sphere-like submanifolds and introduced conditions on external curvature and torsion, which lead to a definition of a rigid sphere.
Abstract
This paper deals with the generalization of usual round spheres in the flat Minkowski spacetime to the case of a generic four-dimensional spacetime manifold $M$. We consider geometric properties of sphere-like submanifolds in $M$ and introduce conditions on external curvature and torsion, which lead to a definition of a {\em rigid sphere}. The main result is a local existence theorem concernig such spheres. For this purpose we apply the surjective implicit function theorem. The proof is based on a detailed analysis of the linearized problem and leads to an eight-parameter family of solutions in case when the metric tensor $g$ of $M$ is from a certain neighbourhood of the flat Minkowski metric. This contribution continues the study of rigid spheres in (Class. Quantum Grav. \textbf{30} (2013), 175010, doi:10.1088/0264-9381/30/17/175010, 18 pp.).

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Local space time constant mean curvature and constant expansion foliations

TL;DR: In this article , a Lyapunov Schmidt reduction is used to construct local foliations of surfaces with prescribed mean curvature, which are then used to characterize the center of mass in general relativity.
References
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Quasi-Local Energy-Momentum and Angular Momentum in GR: A Review Article

TL;DR: The present status of the quasi-local mass-energy-momentum and angular momentum constructions in general relativity is reviewed.
Book

The Evolution Problem in General Relativity

TL;DR: In this paper, the authors propose analytic methods in the initial value problem and estimate the connection coefficients and the curvature tensor tensor for the initial hypersurface and the last slice.
Journal ArticleDOI

A Simple Derivation of Canonical Structure and Quasi-local Hamiltonians in General Relativity

TL;DR: In this article, a new method of variation of the gravitational Lagrangian is proposed, which leads in a simple and straightforward way to the canonical description of the gravity field dynamics in a finite volume V with boundary.
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