2001
DOI: 10.1103/physrevd.63.044015
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Brane-world inflation without inflaton on the brane

Abstract: Inspired by the Randall-Sundrum brane-world scenario, we investigate the possibility of braneworld inflation driven not by an inflaton field on the brane, but by a bulk, dilaton-like gravitational field. As a toy model for the dilaton-like gravitational field, we consider a minimally coupled massive scalar field in the bulk 5-dimensional spacetime, and look for a perturbative solution in the anti-de Sitter (AdS) background. For an adequate range of the scalar field mass, we find a unique solution that has non-… Show more

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Cited by 108 publications
(159 citation statements)
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“…Inflation on the brane has been considered in the literature (see for example [10][11][12][13]), and even the tendency of the brane embedded into AdS bulk to dissipate anisotropy was reported [14,15], but it is not perfectly clear what would happen if the bulk itself was anisotropic (or non-homogeneous, for that matter). Would inflation on the brane be enough to isotropize both the brane and the bulk (which has much larger volume), or would some sort of "bulk inflation" be needed?…”
Section: Discussionmentioning
confidence: 99%
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“…Inflation on the brane has been considered in the literature (see for example [10][11][12][13]), and even the tendency of the brane embedded into AdS bulk to dissipate anisotropy was reported [14,15], but it is not perfectly clear what would happen if the bulk itself was anisotropic (or non-homogeneous, for that matter). Would inflation on the brane be enough to isotropize both the brane and the bulk (which has much larger volume), or would some sort of "bulk inflation" be needed?…”
Section: Discussionmentioning
confidence: 99%
“…A number of cosmological scenarios based on the brane-world concept was explored [5][6][7][8][9], including some models with inflation on the brane [10][11][12][13] and different embedding geometries [14,15].…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, the reheating after inflation based on this scenario has been discussed by Yokoyama and Himemoto [14], and they found that the standard inflationary cosmology is reproduced under the same conditions. However, these results for this new scenario are more or less based on a particular scalar field configuration discussed in [11], the details of which will be explained in the next section. Therefore, strictly speaking, the viability and generality of this scenario should be more carefully examined.…”
Section: Introductionmentioning
confidence: 99%
“…However, in the present spatially homogeneous case, the Bianchi identities supply the evolution equation of E tt on the brane as [11] …”
Section: Braneworld Inflation Without Inflaton On the Branementioning
confidence: 99%
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