Solving the Inverse Problem with Inhomogeneous Universes(Astrophysics and Cosmology)
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概要
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We construct the Lemaitre-Tolman-Bondi (LTB) dust universe whose distance-redshift relation is equivalent to that in the concordance Λ cold dark matter (ΛCDM) cosmological model. In our model, the density distribution and velocity field are not homogeneous, whereas the big-bang time is uniform, which implies that the universe is homogeneous at its beginning. We also study the effects of local clumpiness in the density distribution as well as the effects of large-scale inhomogeneities on the distance-redshift relation, and show that these effects may reduce the amplitude of large-scale inhomogeneities necessary for having a distance-redshift relation that is the same as that of the concordance ΛCDM universe. We also study the temporal variation of the cosmological redshift and show that, by the observation of this quantity, we can distinguish our LTB universe model from the concordance ΛCDM model, even if their redshift-distance relations are equivalent to each other.
- 2008-11-25
著者
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KAI Tomohiro
Department of Physics, Graduate School of Science, Osaka City University
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NAKAO Ken-ichi
Department of Physics, Graduate School of Science, Osaka City University
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YOO Chul-Moon
Department of Physics, Graduate School of Science, Osaka City University
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YOO Chul-Moon
Yukawa Institute for Theoretical Physics, Kyoto University
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Kai Tomohiro
Department Of Physics Graduate School Of Science Osaka City University
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Yoo Chul-moon
Yukawa Institute For Theoretical Physics Kyoto University:asia Pacific Center For Theoretical Physic
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Yoo Chul-moon
Yukawa Institute For Theoretical Physics Kyoto University
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Nakao Ken-ichi
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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Nakao Ken‐ichi
Department Of Physics Graduate School Of Science Osaka City University
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Nakao Ken‐ichi
Department Of Mathematics And Physics Graduate School Of Science Osaka City University
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YOO Chul-Moon
Yukawa Institute for Theoretical Physics, Kyoto University:Asia Pacific Center for Theoretical Physics, Pohang University of Science and Technology
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NAKAO Ken-ichi
Department of Mathematics and Physics, Graduate School of Science, Osaka City University
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