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Looking for an extra dimension with tomographic cosmic shear
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Looking for an extra dimension with tomographic cosmic shear
Yong-Seon Song?
Enrico Fermi Institute, University of Chicago, Chicago IL 60637
(Dated: February 2, 2008)
The cosmic acceleration was discovered in one of the brane-based models. We are interested in
discriminating this model from the dark energy by tomographic cosmic shear. Growth factors are
different in the two models when one adjusts parameters to get nearly identical H(z). The two
models could be distinguished with independent determinations of both geometrical factors and
the growth factor. We introduce new parameterizations to separate the influence of geometry and
the influence of growth on cosmic shear maps. We find that future observations will be able to
distinguish between both models.
PACS numbers: draft
I. INTRODUCTION
The discovery of cosmic acceleration [1, 2, 3] has led
to theoretical efforts to understand the nature of the cos-
mic acceleration [4, 5, 6, 7] and phenomenological efforts
to discriminate the diverse modelings [8, 9, 10, 11, 12,
13, 14]. Most theoretical explanations for the acceler-
ation preserve Einstein gravity and add a new smooth
and dark component called Dark Energy (DE) [4, 5].
However, DE is not yet strongly supported theoretically
nor phenomenologically. The similar cosmic acceleration
was also discovered in one of brane-based models [6] by
C. Deffayet et.al. [15, 16] (hereafter DGP model rep-
resents this discovery of the cosmic acceleration in the
brane-based model [6].)
In the DGP model, the cosmic acceleration is gener-
ated by the modified gravity due to the presence of the
extra dimension in DGP. The study of the extra dimen-
sion physics influencing the DGP model has been inves-
tigated by [17, 18, 19]. Dvali, Gabadadze and Porrati
designed a brane where ordinary matter is embedded in
an infinite extra dimension and gravity is modified at
larger scale [6]. The model (DGP) which generates t
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