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Prog. Theor. Phys. Vol. 120 No. 5 (2008) pp. 937-960
Solving the Inverse Problem with Inhomogeneous Universes
Chul-Moon Yoo,1,3
Tomohiro Kai2 and
Ken-ichi Nakao2
1Yukawa Institute for Theoretical Physics,
Kyoto University, Kyoto 606-8502, Japan
2Department of Physics, Graduate School of Science,
Osaka City University, Osaka 558-8585, Japan
3Asia Pacific Center for Theoretical Physics,
Pohang University of Science and Technology, Pohang 790-784, Korea
(Received July 7, 2008)
Abstract:
We construct the Lemaître-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.
URL :
http://ptp.ipap.jp/link?PTP/120/937/
DOI : 10.1143/PTP.120.937
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