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Quantum Gravity in Large Dimensions

High Energy Physics - Theory 2008-11-26 v1 General Relativity and Quantum Cosmology

Abstract

Quantum gravity is investigated in the limit of a large number of space-time dimensions, using as an ultraviolet regularization the simplicial lattice path integral formulation. In the weak field limit the appropriate expansion parameter is determined to be 1/d1/d. For the case of a simplicial lattice dual to a hypercube, the critical point is found at kc/λ=1/dk_c/\lambda=1/d (with k=1/8πGk=1/8 \pi G) separating a weak coupling from a strong coupling phase, and with 2d22 d^2 degenerate zero modes at kck_c. The strong coupling, large GG, phase is then investigated by analyzing the general structure of the strong coupling expansion in the large dd limit. Dominant contributions to the curvature correlation functions are described by large closed random polygonal surfaces, for which excluded volume effects can be neglected at large dd, and whose geometry we argue can be approximated by unconstrained random surfaces in this limit. In large dimensions the gravitational correlation length is then found to behave as log(kck)1/2| \log (k_c - k) |^{1/2}, implying for the universal gravitational critical exponent the value ν=0\nu=0 at d=d=\infty.

Keywords

Cite

@article{arxiv.hep-th/0512003,
  title  = {Quantum Gravity in Large Dimensions},
  author = {Herbert W. Hamber and Ruth M. Williams},
  journal= {arXiv preprint arXiv:hep-th/0512003},
  year   = {2008}
}

Comments

47 pages, 2 figures