Eddington’s Prediction for General Relativity Revisited


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Eddington’s prediction for general relativity (GR) is exemplified by three cases: a static spherically symmetric gravitational field, radiation of gravitational waves, and a homogeneous isotropic cosmological model. The results of GR for a static field are obtained using only Poisson’s equation instead of the Einstein–Hilbert equations. Degeometrization of GR will allow the gravitational interaction to be unified with others described in the framework of the Standard Model of particle physics.

作者简介

M. Fil’chenkov

Institute of Gravitation and Cosmology, RUDN University

编辑信件的主要联系方式.
Email: fmichael@mail.ru
俄罗斯联邦, ul. Miklukho-Maklaya 6, Moscow, 117198

Yu. Laptev

Institute of Gravitation and Cosmology, RUDN University

Email: fmichael@mail.ru
俄罗斯联邦, ul. Miklukho-Maklaya 6, Moscow, 117198

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