2000
DOI: 10.1088/1126-6708/2000/09/012
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A critical cosmological constant from millimeter extra dimensions

Abstract: We consider 'brane universe' scenarios with standard-model fields localized on a 3-brane in 6 spacetime dimensions. We show that if the spacetime is rotationally symmetric about the brane, local quantities in the bulk are insensitive to the couplings on the brane. This potentially allows compactifications where the effective 4-dimensional cosmological constant is independent of the couplings on the 3-brane. We consider several possible singularity-free compactification mechanisms, and find that they do not mai… Show more

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Cited by 178 publications
(269 citation statements)
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References 16 publications
(41 reference statements)
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“…For α i > 1, ζ and the warp factor are discontinuous around z i . Moreover, for α i < −1, there exists 2 We note that in Romans supergravity [15], the scalar potential is negative definite with g 2 → −g 2 in our setup. In this case, there exists only one real root of P (W ) so the value of W is not bounded.…”
Section: The General Warped Solutionmentioning
confidence: 70%
“…For α i > 1, ζ and the warp factor are discontinuous around z i . Moreover, for α i < −1, there exists 2 We note that in Romans supergravity [15], the scalar potential is negative definite with g 2 → −g 2 in our setup. In this case, there exists only one real root of P (W ) so the value of W is not bounded.…”
Section: The General Warped Solutionmentioning
confidence: 70%
“…Although it remains an unsolved problem as to how this dynamics works in string theory, the effects of on-brane loops [83][84][85][86] and back-reaction [26,27,[87][88][89][90] have been studied for non-supersymmetric, codimension-2 branes in simpler 6D extra-dimensional models. These simpler systems resemble their 10D cousins in that the back-reaction is also competitive with bulk physics in stabilising the extra dimensions, yet doesn't destroy the presence of large-volume solutions.…”
Section: Modulus Spectrum and Couplings: Correctionsmentioning
confidence: 99%
“…is the spin-summed Standard Model Higgs amplitude squared, p j represent the neutron four-momenta, and everything else maintains its old definition, except that it is now appropriate to use Maxwell-Boltzman distributions for the non-relativistic neutrons with number density n N 61) and in the phase space measures E j → m N , where m N is the nucleon mass.…”
Section: Nucleon-bulk Bremsstrahlung In Supernovaementioning
confidence: 99%
“…For illustrative purposes (following the discussion of [14]) we do so here ignoring the energetics of the gravitational back-reaction of the branes. This is known not to be a good approximation in general for codimension-2 objects since in many cases it is the classical bulk back-reaction that cancels the brane tensions to allow the classical brane geometries to be flat [24,30,61]. (Indeed, it is this property -together with bulk supersymmetry -that underlies their use as a starting point for seeking solutions to the cosmological constant problem [25,27,62].)…”
Section: B Probe-brane Energeticsmentioning
confidence: 99%