Higher order corrections to the Newtonian potential in the Randall-Sundrum model
arXiv:hep-ph/0403302 · doi:10.1103/PhysRevD.70.104009
Abstract
The general formalism for calculating the Newtonian potential in fine-tuned or critical Randall-Sundrum braneworlds is outlined. It is based on using the full tensor structure of the graviton propagator. This approach avoids the brane-bending effect arising from calculating the potential for a point source. For a single brane, this gives a clear understanding of the disputed overall factor 4/3 entering the correction. The result can be written on a compact form which is evaluated to high accuracy for both short and large distances.
12 pages, LaTeX2e with RevTeX4, 3 postscript figures; Minor corrections, references updated
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