2007
DOI: 10.1103/physrevd.76.124009
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Regularized braneworlds of arbitrary codimension

Abstract: We consider a thick p-brane embedded in an n-dimensional spacetime possessing radial symmetry in the directions orthogonal to the brane. We first consider a static brane, and find a general fine tuning relationship between the brane and bulk parameters required for the brane to be flat. We then consider the cosmology of a time dependent brane in a static bulk, and find the Friedmann equation for the brane scale factor a(t). The singularities that would ordinarily arise when considering arbitrary codimensions a… Show more

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Cited by 29 publications
(31 citation statements)
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“…A similar caveat applies to models with exponential rather than power law suppression of the field with curvature (e.g. [22]). …”
Section: A Modelsmentioning
confidence: 99%
“…A similar caveat applies to models with exponential rather than power law suppression of the field with curvature (e.g. [22]). …”
Section: A Modelsmentioning
confidence: 99%
“…This is known as the Chameleon mechanism [7]. In the context of f (R) gravity, by tuning the function f , it is possible to make the Compton wavelength of the BD scalar short at solar system scales and screen the BD scalar interaction [10][11][12][13].…”
Section: Introductionmentioning
confidence: 99%
“…Nevertheless, some viable f (R) models have been proposed, which are capable of reproducing a realistic cosmological evolution, and prevent violations of local gravitational tests and instabilities in the presence of matter distributions (see Refs. [15,16,17]), and even to reproduce the inflationary phase (see Ref. [18]).…”
Section: Introductionmentioning
confidence: 99%