Quasi-local energy from a Minkowski reference

被引:8
|
作者
Chen, Chiang-Mei [1 ,2 ]
Liu, Jian-Liang [3 ,4 ]
Nester, James M. [1 ,5 ,6 ]
机构
[1] Natl Cent Univ, Dept Phys, Chungli 32001, Taiwan
[2] Natl Cent Univ, Ctr High Energy & High Field Phys CHiP, Chungli 32001, Taiwan
[3] Dongguan Univ Technol, Dept Math & Data Sci, Dongguan, Peoples R China
[4] Shantou Univ, Dept Math, Shantou 515063, Guandong, Peoples R China
[5] Natl Cent Univ, Grad Inst Astron, Chungli 32001, Taiwan
[6] Natl Taiwan Univ, Leung Ctr Cosmol & Particle Astrophys, Taipei 10617, Taiwan
基金
中国国家自然科学基金; 中国博士后科学基金;
关键词
Hamiltonian; Quasi-local energy; Minkowski reference; GRAVITATIONAL ENERGY; CONSERVATION-LAWS; ANGULAR-MOMENTUM; GENERAL-RELATIVITY; LOCALIZATION; POSITIVITY; SYSTEM; MASS;
D O I
10.1007/s10714-018-2484-z
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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 quasi-local (associated with a closed 2-surface). Here we consider quasi-local proposals (including pseudotensors) in the Lagrangian-Noether-Hamiltonian formulations. There are two ambiguities: (1) there are many possible expressions, (2) they depend on some non-dynamical structure, e.g., a reference frame. The Hamiltonian approach gives a handle on both problems. The Hamiltonian perspective helped us to make a remarkable discovery: with an isometric Minkowski reference a large class of expressionsnamely all those that agree with the Einstein pseudotensor's Freud superpotential to linear ordergive a common quasi-local energy value. Moreover, with a best-matched reference on the boundary this is the Wang-Yau mass value.
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页数:14
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