arXiv Analytics

Sign in

arXiv:hep-ph/9904267AbstractReferencesReviewsResources

Cosmological Constraints on Theories with Large Extra Dimensions

Lawrence J. Hall, David Smith

Published 1999-04-08, updated 1999-04-23Version 2

In theories with large extra dimensions, constraints from cosmology lead to non-trivial lower bounds on the fundamental scale M_F, corresponding to upper bounds on the radii of the compact extra dimensions. These constraints are especially relevant to the case of two extra dimensions, since only if M_F is 10 TeV or less do deviations from the standard gravitational force law become evident at distances accessible to planned sub-mm gravity experiments. By examining the graviton decay contribution to the cosmic diffuse gamma radiation, we derive, for the case of two extra dimensions, a conservative bound M_F > 110 TeV, corresponding to r_2 < 5.1 times 10^-5 mm, well beyond the reach of these experiments. We also consider the constraint coming from graviton overclosure of the universe and derive an independent bound M_F > 6.5 h^(-1/2) TeV, or r_2 < .015 h mm.

Related articles: Most relevant | Search more
arXiv:hep-ph/0101131 (Published 2001-01-12, updated 2001-03-15)
Cosmological Constraints on Large Extra Dimensions
arXiv:1704.06663 [hep-ph] (Published 2017-04-21)
A scale at 10 MeV, gravitational topological vacuum, and large extra dimensions
arXiv:hep-ph/0001126 (Published 2000-01-14)
Cosmological Constraints on the MSSM