Quasilocal conservation laws: why we need them

DOI10.1088/0264-9381/29/21/215012zbMath1266.83068arXiv1206.6512OpenAlexW3099642939WikidataQ60721098 ScholiaQ60721098MaRDI QIDQ4920163

Paul L. McGrath, Richard J. Epp, Robert B. Mann

Publication date: 16 May 2013

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1206.6512

zbMATH Keywords

gravitational effectselectromagnetic Poynting fluxgravitational energy fluxquasilocal conservation laws

Mathematics Subject Classification ID

Gravitational energy and conservation laws; groups of motions (83C40) Electromagnetic theory (general) (78A25) Equations of motion in general relativity and gravitational theory (83C10)

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Relativistic rigid systems and the cosmic expansion ⋮ Energy of cosmological spacetimes and perturbations: a quasilocal approach ^* ⋮ Quasilocal conservation laws in cosmology: A first look

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