Hamilton-Jacobi Equation for Brans-Dicke Theory and Its Long-Wavelength Solution : Astrophysics and Relativity
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概要
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The Hamilton-Jacobi equation for the Brans-Dicke theory is solved by using a long-wavelength approximation. We examine the non-linear evolution of the inhomogeneities in the dust fluid case and the cosmological constant case. In the case of dust fluid, it turns out that the inhomogeneities of space-time grow. In the case of cosmological constant, the inhomogeneities decay, which is consistent with the cosmic no hair conjecture. The inhomogeneities of the density perturbation and the gravitational constant behave in a manner similar to those of space-time.
- 理論物理学刊行会の論文
- 1995-11-25
著者
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SODA Jiro
Department of Physics, Kyoto University
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Soda Jiro
Department Of Fundamental Sciences Fihs Kyoto University
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Soda Jiro
Reaearch Institute For Theoretical Physics Hiroshima University
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ISHIHARA Hideki
Department of Physics, Tokyo Institute of Technology
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IGUCHI Osamu
Department of Physics, Tokyo Institute of Technology
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Iguchi Osamu
Department Of Physics Ochanomizu University
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Ishihara Hideki
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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Ishihara Hideki
Department Of Physics Tokyo Institute Of Technology
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ISHIHARA Hideki
Department of Physics, Nagoya University
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