Weinberg's energy-momentum pseudotensor for Schwarzschild field

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dc.creatorNikishov, A. I.
dc.date2000-02-10
dc.date.accessioned2026-07-07T03:24:45Z
dc.date.available2026-07-07T03:24:45Z
dc.descriptionWeinberg's energy-momentum pseudotensor is obtained for Schwarzschild metric in harmonic coordinates. On the horizon it possesses unintegrable singularities. For this reason the total energy of a collapsar can't be obtained by integrating energy density over the system's volume. The implication for gravity theories is noted. A thought on how to choose unique energy-momentum tensor is given.
dc.description5 pages, Latex, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/0002038
dc.identifierhttp://arxiv.org/abs/gr-qc/0002038
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33456
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleWeinberg's energy-momentum pseudotensor for Schwarzschild field
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