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Related papers: A spinorial quasilocal mass

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Motivated by the important work of Brown adn York on quasilocal energy, we propose definitions of quasilocal energy and momentum surface energy of a spacelike 2-surface with positive intrinsic curvature in a spacetime. We show that the…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Chiu-Chu Melissa Liu , Shing-Tung Yau

We prove the following stronger verson of the positivity of quasi-local mass stated in gr-qc/0303019: the quasi-local energy (mass) of each connected component of the boundary of a compact spacelike hypersurface which satisfies the local…

Differential Geometry · Mathematics 2007-05-23 Chiu-Chu Melissa Liu , Shing-Tung Yau

We discuss the concepts of energy and mass in relativity. On a finitely extended spatial region, they lead to the notion of quasilocal energy/mass for the boundary 2-surface in spacetime. A new definition was found in [27] that satisfies…

General Relativity and Quantum Cosmology · Physics 2012-11-08 Mu-Tao Wang

We first describe a class of spinor-curvature identities (SCI) which have gravitational applications. Then we sketch the topic of gravitational energy-momentum, its connection with Hamiltonian boundary terms and the issues of positivity and…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Chiang-Mei Chen , James M. Nester , Roh-Suan Tung

The Hamiltonian of a gravitational system defined in a region with boundary is quantized. The classical Hamiltonian, and starting point for the regularization, is required by functional differentiablity of the Hamiltonian constraint. The…

General Relativity and Quantum Cosmology · Physics 2009-10-31 Seth A. Major

The classical value of the Hamiltonian for a system with timelike boundary has been interpreted as a quasilocal energy. This quasilocal energy is not positive definite. However, we derive a `quasilocal dominant energy condition' which is…

General Relativity and Quantum Cosmology · Physics 2009-10-22 Geoff Hayward

From a covariant Hamiltonian formulation, using symplectic ideas, we obtain covariant quasilocal energy-momentum boundary expressions for general gravity theories. The expressions depend upon which variables are fixed on the boundary, a…

General Relativity and Quantum Cosmology · Physics 2009-10-22 Chiang-Mei Chen , James M. Nester , Roh Suan Tung

The quasilocal energy of gravitational and matter fields in a spatially bounded region is obtained by employing a Hamilton-Jacobi analysis of the action functional. First, a surface stress-energy-momentum tensor is defined by the functional…

General Relativity and Quantum Cosmology · Physics 2008-11-26 J. David Brown , James W. York

The specification of energy for gravitating systems has been an unsettled issue since Einstein proposed his pseudotensor. It is now understood that energy-momentum is \emph{quasi-local} (associated with a closed 2-surface). Here we consider…

General Relativity and Quantum Cosmology · Physics 2018-11-15 Chiang-Mei Chen , Jian-Liang Liu , James M. Nester

We study the quasi-local masses arising in general relativity using spinors and prove their positivity property. This leads to the question of a pure quasi-local proof of the positivity of the Wang-Yau \cite{yau} quasi-local mass. More…

Mathematical Physics · Physics 2024-09-20 Puskar Mondal , Shing-Tung-Yau

Early energy-momentum investigations for gravitating systems gave reference frame dependent pseudotensors; later the quasilocal idea was developed. Quasilocal energy-momentum can be determined by the Hamiltonian boundary term, which also…

General Relativity and Quantum Cosmology · Physics 2009-10-31 C. C. Chang , J. M. Nester , C. M. Chen

This paper investigates the relationship between the quasilocal energy of Brown and York and certain spinorial expressions for gravitational energy constructed from the Witten-Nester integral. A key feature of the Brown-York method for…

General Relativity and Quantum Cosmology · Physics 2010-04-06 Stephen R. Lau

We modify previous quasi-local mass definition. The new definition provides expressions of the quasi-local energy, the quasi-local linear momentum and the quasi-local mass. And they are equal to the ADM expressions at spatial infinity.…

General Relativity and Quantum Cosmology · Physics 2009-12-15 Xiao Zhang

We present two complementary approaches for determining the reference for the covariant Hamiltonian boundary term quasi-local energy and test them on spherically symmetric spacetimes. On the one hand, we isometrically match the 2-surface…

General Relativity and Quantum Cosmology · Physics 2015-06-05 Ming-Fan Wu , Chiang-Mei Chen , Jian-Liang Liu , James M. Nester

Witten's proof for the positivity of the ADM mass gives a definition of energy in terms of three-surface spinors. In this paper, we give a generalisation for the remaining six Poincar\'e charges at spacelike infinity, which are the angular…

General Relativity and Quantum Cosmology · Physics 2017-02-14 Wolfgang Wieland

A quasi-local energy for Einstein's general relativity is defined by the value of the preferred boundary term in the covariant Hamiltonian formalism. The boundary term depends upon a choice of reference and a time-like displacement vector…

General Relativity and Quantum Cosmology · Physics 2015-05-28 Jian-Liang Liu , Chiang-Mei Chen , James M Nester

The quasilocal energy associated with a constant stationary time slice of the Kerr spacetime is presented. The calculations are based on a recent proposal \cite{by} in which quasilocal energy is derived from the Hamiltonian of spatially…

General Relativity and Quantum Cosmology · Physics 2009-10-22 Erik A. Martinez

We show that the quantization of energy for Willmore spheres into closed Riemannian manifolds holds provided that the Willmore energy and the area are uniformly bounded. The analogous energy quantization result holds for Willmore surfaces…

Analysis of PDEs · Mathematics 2021-12-28 Alexis Michelat , Andrea Mondino

In this paper, we obtain lower bounds for the Brown-York quasilocal mass and the Bartnik quasilocal mass for compact three manifolds with smooth boundaries. As a consequence, we derive sufficient conditions for the existence of horizons for…

Differential Geometry · Mathematics 2007-05-23 Yuguang Shi , Luen-Fai Tam

A quasi-local mass, typically defined as an integral over a spacelike $2$-surface $\Sigma$, should encode information about the gravitational field within a finite, extended region bounded by $\Sigma$. Therefore, in attempts to quantize…

General Relativity and Quantum Cosmology · Physics 2024-07-16 Bowen Zhao , Shing-Tung Yau , Lars Andersson
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