Linear Bimetric Gravitation Theory

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dc.creatorIonescu-Pallas, N.
dc.creatorPiso, M. I.
dc.creatorOnofrei, S.
dc.date1994-07-14
dc.date.accessioned2026-07-07T03:30:24Z
dc.date.available2026-07-07T03:30:24Z
dc.descriptionA general bimetric theory of gravitation is described as a linear in the second approximation. This is allowed due to the small experimental significance of the higher order terms. Solar System tests are satisfied. The theory allows black holes, which are physical singularities. The predicted black hole radius is equal to the one resulting from Einstein's theory, if the compatibility between the gauge conditions and the existence of gravitational waves is required (the Rosen-Fock metric). The quadrupolar gravitational radiation formula is regained.
dc.descriptionGravitational Res. Lab. Bucharest preprint GRL-04-94
dc.identifierhttps://arxiv.org/abs/gr-qc/9407017
dc.identifierhttp://arxiv.org/abs/gr-qc/9407017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35522
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleLinear Bimetric Gravitation Theory
dc.typetext

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