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arxiv: 1811.05640 · v1 · pith:CTBF5C7Anew · submitted 2018-11-14 · 🌀 gr-qc · hep-th

Quasi-local energy from a Minkowski reference

classification 🌀 gr-qc hep-th
keywords quasi-localreferenceenergyeinsteinhamiltonianminkowskipseudotensorthere
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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 quasi-local proposals (including pseudotensors) in the Lagrangian-Noether-Hamiltonian formulations. There are two ambiguities: (i) there are many possible expressions, (ii) 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 expressions---namely all those that agree with the Einstein pseudotensor's Freud superpotential to linear order---give 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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