Papapetrou Energy-Momentum Tensor for Chern-Simons Modified Gravity

dc.creatorGuarrera, David
dc.creatorHariton, A. J.
dc.date2007-02-05
dc.date2007-11-16
dc.date.accessioned2026-07-07T11:01:41Z
dc.date.available2026-07-07T11:01:41Z
dc.descriptionWe construct a conserved, symmetric energy-momentum (pseudo-)tensor for Chern-Simons modified gravity, thus demonstrating that the theory is Lorentz invariant. The tensor is discussed in relation to other gravitational energy-momentum tensors and analyzed for the Schwarzschild, Reissner-Nordstrom, and FRW solutions. To our knowledge this is the first confirmation that the Reissner-Nordstrom and FRW metrics are solutions of the modified theory.
dc.description8 pages; typos corrected, references fixed, some calculations shortened
dc.identifierhttps://arxiv.org/abs/gr-qc/0702029
dc.identifierhttp://arxiv.org/abs/gr-qc/0702029
dc.identifierPhys.Rev.D76:044011,2007
dc.identifierdoi:10.1103/PhysRevD.76.044011
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188022
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titlePapapetrou Energy-Momentum Tensor for Chern-Simons Modified Gravity
dc.typetext

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