K. Hayashi, T. Shirafuji
Abstract
New general relativity predicts a static, isotropic spacetime quite different from the Schwarzschild spacetime of general relativity, unless one of the two unknown parameters, ε, is exactly zero. In this paper we study its structure as a Riemannian spacetime, paying special attentions to motions of test particles therein.
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New general relativity predicts a static, isotropic spacetime quite different from the Schwarzschild spacetime of general relativity, unless one of the two unknown parameters, ε, is exactly zero. In this paper we study its structure as a Riemannian spacetime, paying special attentions to motions of test particles therein.
Key concepts: Physics, Spacetime, Spherically symmetric spacetime, General relativity, Stationary spacetime, Mathematics of general relativity, Isotropy, Classical mechanics