The cosmological constant problem in codimension-two brane models
arXiv:hep-th/0508065 · doi:10.1016/j.physletb.2005.09.042
Abstract
We discuss the possibility of a dynamical solution to the cosmological constant problem in the contaxt of six-dimensional Einstein-Maxwell theory. A definite answer requires an understanding of the full bulk cosmology in the early universe, in which the bulk has time-dependent size and shape. We comment on the special properties of codimension two as compared to higher codimensions.
11 pages
References in corpus (18)
- Cosmology and the Fate of Dilatation Symmetry
- Towards a Naturally Small Cosmological Constant from Branes in 6D Supergravity
- Einstein gravity on the codimension 2 brane?
- Can codimension-two branes solve the cosmological constant problem?
- Cosmology of codimension-two braneworlds
- Selftuning and its footprints
- Spheres, Deficit Angles and the Cosmological Constant
- A Conical Tear Drop as a Vacuum-Energy Drain for the Solution of the Cosmological Constant Problem
- Football Shaped Extra Dimensions and the Absence of Self-Tuning
- Gravity on codimension 2 brane worlds
- Codimension-two branes in six-dimensional supergravity and the cosmological constant problem
- A comment on the self-tuning of cosmological constant with deficit angle on a sphere
- 4d-Flat Compactifications With Brane Vorticities
- Brane solutions of a spherical sigma model in six dimensions
- Gravitational Perturbations of a Six Dimensional Self-Tuning Model
- Nonsingular 4d-flat branes in six-dimensional supergravities
- Holographic Branes
- Codimension Two Branes in Einstein-Gauss-Bonnet Gravity
Cited by in corpus (9)
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- Braneworlds in six dimensions: new models with bulk scalars
- Gravitational Waves in a Codimension Two Braneworld
- The Effective Field Theory of Codimension-two Branes
- The consistency of codimension-2 braneworlds and their cosmology
- Models of modified and cuscuton braneworld
- Constraints for warped branes