Prog. Theor. Phys. Vol. 84 No. 1 (1990) pp. 36-40
Static, Isotropic Spacetime in New General Relativity
Institute of Physics, Kitasato University, Sagamihara 228
*Physics Department, Saitama University, Urawa 338
(Received March 29, 1990)
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.
DOI : 10.1143/PTP.84.36
- T. Kawai and N. Toma, Prog. Theor. Phys. 83 (1990), 1[PTP].
K. Hayashi and T. Shirafuji, Phys. Rev. D19 (1979), 3524[APS]. Earlier references are quoted therein.
- See, for example, C. W. Misner, K. S. Thorne and J. A. Wheeler, Gravitation (Freeman, San Francisco, 1973), chap. 31.
- For the Penrose diagram, see, for example, S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time (Cambridge Univ. Press, Cambridge, 1973), chap. 5.
Citing Article(s) :
Progress of Theoretical Physics Vol. 96 No. 5 (1996) pp. 933-947
Equivalence Principle in the New General Relativity
Takeshi Shirafuji, Gamal G.L. Nashed and Yoshimitsu Kobayashi