Covariant Energy-Momentum Conservation In General Relativity

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dc.creatorGibbs, Philip E.
dc.date1997-01-08
dc.date1997-01-17
dc.date.accessioned2026-07-07T08:59:36Z
dc.date.available2026-07-07T08:59:36Z
dc.descriptionA covariant formula for conserved currents of energy, momentum and angular-momentum is derived from a general form of Noethers theorem applied directly to the Einstein-Hilbert action of classical general relativity. Energy conservation in a closed big-bang cosmology is discussed as a special case. Special care is taken to distinguish between kinematic and dynamic expressions.
dc.description12 pages, postscript, no figures, references added
dc.identifierhttps://arxiv.org/abs/gr-qc/9701028
dc.identifierhttp://arxiv.org/abs/gr-qc/9701028
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/147773
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCovariant Energy-Momentum Conservation In General Relativity
dc.typetext

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