On a possibility of scalar gravitational wave detection from the binary pulsar PSR 1913 +16

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dc.creatorBaryshev, Yurij V.
dc.date1999-11-22
dc.date.accessioned2026-07-07T03:33:43Z
dc.date.available2026-07-07T03:33:43Z
dc.descriptionIt is shown that detecting or setting an upper limit on the scalar gravitational radiation is a good experimental test of relativistic gravity theories. The relativistic tensor-field theory of gravitation is revised and it is demonstrated that the scalar monopole gravitational radiation must be added to the usual quadrupole radiation. In the case of the binary pulsar PSR 1913+16 it is predicted the existence 0.735 % excess of the gravitational radiation due to the scalar gravitational waves.
dc.description10 pages, no figures
dc.identifierhttps://arxiv.org/abs/gr-qc/9911081
dc.identifierhttp://arxiv.org/abs/gr-qc/9911081
dc.identifierProceeding of the First Edoardo Amaldi Conference on "Gravitational Wave Experiments", eds. E.Coccia, G.Pizzella, F.Ronga, World Scientific Publ.Co., 1995, pp.251-260
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36686
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectQuantum Physics
dc.titleOn a possibility of scalar gravitational wave detection from the binary pulsar PSR 1913 +16
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