Quantum Theory of Gravity and the Perihelion Motion of the Mercury
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概要
- 論文の詳細を見る
In the quantum theory of gravity the potential between two celestial bodies is calculated up to order (υ/c)^2 by treating the celestial bodies as assemblies of nucleons. It is necessary to calculate three-body potentials in order to get the potential proportional to G^2,G being the gravitational constant. A method is discussed for determing the retarded potential uniquely. The potential obtained coincides with the classical one given by Einstein, Infeld and Hoffman. The perihelion motion of the Mercury is also discussed.
- 理論物理学刊行会の論文
- 1971-11-25
著者
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Hiida Kichiro
Institute For Nuclear Study University Of Tokyo
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Kikugawa Masayoshi
Institute For Nuclear Study University Of Tokyo : The Department Of Physics Hiroshima University
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Hiida Kichiro
Institute For Nuclear Study Tokyo University
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KIKUGAWA Masayoshi
Institute for Nuclear Study, University of Tokyo : the Department of Physics, Hiroshima University
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- Substitution Law and Identity for Long-Range Potentials
- General Theory of Chiral Transformations
- Gravitation Physics
- Einstein's Theory of Relativity and Mach's Principle
- Coordinate Condition and Higher Order Gravitational Potential in Canonical Formalism
- A Theory of Anomalous Gravitational Interaction. I : Case of the Bose Particle
- Quantum Theory of Gravity and the Perihelion Motion of the Mercury
- Gauge Transformation and Gravitational Potentials
- Perturbation Calculation of Gravitational Potentials
- Chiral Symmetry in the Unified Fermion Theory. I : SU(2)×SU(2)