On a nonlinear and lorentz-invariant version of newtonian gravitation

dc.contributor.authorRawal, J. J.
dc.contributor.authorNarlikar, J. V.
dc.date.accessioned2012-03-24T10:02:19Z
dc.date.available2012-03-24T10:02:19Z
dc.date.issued1982-08-02
dc.description.abstractThe Newtonian theory of gravitation is modified to include the gravitational energy as a source of gravitational potential, thus making the theory self-coupled and nonlinear. The modified theory can be derived from a Lorentz-invariant action principle. The Kepler problem is discussed in this theory and it is shown that the perihelion of the orbit steadily precesses. The rate of precession is, however, insufficient to account for the observed precession of the perihelion of Mercury. The differences from the Newtonian theory for the bending of light and the gravitational redshift of spectral lines are shown to be marginal.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1581
dc.language.isoenen_US
dc.publisherIndian Academy of Sciencesen_US
dc.relation.ispartofseriesJournal of Astrophysics and Astronomy;Vol. 3, 1982
dc.subjectNewtonian gravitationen_US
dc.subjectLorentz-invariant generalizationen_US
dc.titleOn a nonlinear and lorentz-invariant version of newtonian gravitationen_US
dc.typeArticleen_US

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