Induced gravity on intersecting brane-worlds Part I: Maximally symmetric solutions
arXiv:0712.0385 · doi:10.1103/PhysRevD.77.084006
Abstract
We explore models of intersecting brane-worlds with induced gravity terms on codimension one branes and on their intersection. Maximally symmetric solutions for the branes and the intersection are found. We find new self-accelerating solutions. In a 6d spacetime, the solutions realize the see-saw modification of gravity where the UV scale of the modification to 4d gravity is determined by 6d Planck scale given by eV and the IR scale of the modification is determined by GeV where is present-day Hubble scale. We find that it is increasingly difficult to construct phenomenologically viable models in higher-dimensional spacetime due to the necessity to have the lower value for the fundamental Planck scale to realize the late time acceleration. It is found that the system also admits self-tuning solutions where the tension at the intersection does not change the geometry of the intersection. The induced gravity terms can avoid the necessity to compactify the extra dimensions. Finally, we discuss the possibility to have ordinary matter at the intersection, without introducing any regularisation, using the induced gravity terms.
16 pages, some mistakes in the identification of the higher codimensional singular structure corrected. Main results unchanged
References in corpus (10)
- Cascading DGP
- Ghosts in the self-accelerating universe
- Sidestepping the Cosmological Constant with Football-Shaped Extra Dimensions
- Non-linear interactions in a cosmological background in the DGP braneworld
- Induced cosmology on a regularized brane in six-dimensional flux compactification
- Cosmological evolution of regularized branes in 6D warped flux compactifications
- The Effective Field Theory of Codimension-two Branes
- Bubbles in the Self-Accelerating Universe
- Brane Induced Gravity: Codimension-2
- A New Dimension Hidden in the Shadow of a Wall