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Prog. Theor. Phys. Vol. 105 No. 4 (2001) pp. 591-606
Radion on the de Sitter Brane
Uchida Gen1,2 and
Misao Sasaki2
1Department of Earth and Space Science, Graduate School of Science
Osaka University, Toyonaka 560-0043, Japan
2Department of Physics, School of Science
University of Tokyo, Tokyo 113-0033, Japan
(Received December 6, 2000)
Abstract:
The radion on the de Sitter brane is investigated at the linear
perturbation level, using the covariant curvature tensor formalism
developed by Shiromizu, Maeda and Sasaki.[SMS]
It is found that if there is
only one de Sitter brane with positive tension, there is no radion, and
thus ordinary Einstein gravity is recovered on the brane, with the
exception of
corrections due to the massive Kaluza-Klein modes.
As a by-product of the covariant curvature tensor formalism,
it is immediately seen that cosmological scalar, vector and tensor
type perturbations all have the same Kaluza-Klein spectrum.
On the other hand, if there are two branes, one with positive tension
and another with negative tension, the gravity on each brane receives corrections from the
radion mode in addition to the Kaluza-Klein modes, and the radion is
found to have a negative mass-squared proportional to the curvature
of the de Sitter brane. This is in contrast to the flat brane case, in which
the radion mass vanishes and becomes degenerate with the 4-dimensional
graviton modes.
To relate our result with the metric perturbation approach,
we derive the second-order action for the brane displacement.
We find that the radion identified in our approach indeed corresponds to
the relative displacement of the branes in the Randall-Sundrum gauge
and describes the scalar curvature perturbations of the branes
in Gaussian normal coordinates around the branes.
The implications of our results with regard to the inflationary brane
universe are briefly discussed.
URL :
http://ptp.ipap.jp/link?PTP/105/591/
DOI : 10.1143/PTP.105.591
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