Higher order corrections to the Newtonian potential in the Randall-Sundrum model

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dc.creatorCallin, Petter
dc.creatorRavndal, Finn
dc.date2004-03-31
dc.date2004-11-11
dc.date.accessioned2026-07-07T03:52:18Z
dc.date.available2026-07-07T03:52:18Z
dc.descriptionThe 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.
dc.description12 pages, LaTeX2e with RevTeX4, 3 postscript figures; Minor corrections, references updated
dc.identifierhttps://arxiv.org/abs/hep-ph/0403302
dc.identifierhttp://arxiv.org/abs/hep-ph/0403302
dc.identifierPhys.Rev. D70 (2004) 104009
dc.identifierdoi:10.1103/PhysRevD.70.104009
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/43413
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHigher order corrections to the Newtonian potential in the Randall-Sundrum model
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