Running with rugby balls: bulk renormalization of codimension-2 branes

• Published in: The journal of high energy physics 2013-01, Vol.2013 (1), p.1-77, Article 102
• Main Authors: Williams, M., Burgess, C. P., van Nierop, L., Salvio, A.
• Format: Article
• Language: English
• Subjects: Boundary conditions; Branes; Classical and Quantum Gravitation; Cosmological constant; Elementary Particles; Hierarchies; High energy physics; Mathematical models; Physics; Physics and Astronomy; Quantum Field Theories; Quantum Field Theory; Quantum Physics; Relativity Theory; Running; String Theory; Two dimensional
• ISSN: 1029-8479; 1029-8479
• DOI: 10.1007/JHEP01(2013)102

A bstract We compute how one-loop bulk effects renormalize both bulk and brane effective interactions for geometries sourced by codimension-two branes. We do so by explicitly integrating out spin-zero, -half and -one particles in 6-dimensional Einstein-Maxwell-Scalar theories compactified to 4 dimensions on a flux-stabilized 2D geometry. (Our methods apply equally well for D dimensions compactified to D − 2 dimensions, although our explicit formulae do not capture all divergences when D > 6.) The renormalization of bulk interactions are independent of the boundary conditions assumed at the brane locations, and reproduce standard heat-kernel calculations. Boundary conditions at any particular brane do affect how bulk loops renormalize this brane’s effective action, but not the renormalization of other distant branes. Although we explicitly compute our loops using a rugby ball geometry, because we follow only UV effects our results apply more generally to any geometry containing codimension-two sources with conical singularities. Our results have a variety of uses, including calculating the UV sensitivity of one-loop vacuum energy seen by observers localized on the brane. We show how these one-loop effects combine in a surprising way with bulk back-reaction to give the complete low-energy effective cosmological constant, and comment on the relevance of this calculation to proposed applications of codimension-two 6D models to solutions of the hierarchy and cosmological constant problems.