Gravity and the Newtonian limit in the Randall-Sundrum model
arXiv:hep-th/0001013 · doi:10.1016/S0370-2693(00)00140-4
Abstract
We point out that the gravitational evolution equations in the Randall-Sundrum model appear in a different form than hitherto assumed. As a consequence, the model yields a correct Newtonian limit in a novel manner.
9 pages, LaTeX, sign changed and references added. We have also appended a remark on the compatibility of the 4D Poincare invariant metric of Randall and Sundrum with the boundary equations
Cited by in corpus (17)
- Radion Dynamics and Electroweak Physics
- Brane worlds
- Gravitational potential correction with Gauss-Bonnet interaction
- Recovery of the Schwarzschild Metric in Theories with Localized Gravity Beyond Linear Order
- Consistent Linearized Gravity in Brane Backgrounds
- Geodesics and Newton's Law in Brane Backgrounds
- Resource Letter on geometrical results for Embeddings and Branes
- Experimental Probes of the Randall-Sundrum Infinite Extra Dimension
- Linearized Analysis of the Dvali-Gabadadze-Porrati Brane Model
- Which action for brane worlds?
- Linearized Gravity in Isotropic Coordinates in the Brane World
- Brane-World charges
- Machine learning applications in astrophysics: Photometric redshift estimation
- A photon mass on the brane
- Probing Short Gravity using Temporal Lensing
- Comments on conformal stability of brane-world models
- Proposed experimental test of Randall-Sundrum Models