The UV behavior of Gravity at Large N

Simple item page
dc.creatorCanfora, F.
dc.date2006-08-29
dc.date2006-09-11
dc.date.accessioned2026-07-07T07:20:30Z
dc.date.available2026-07-07T07:20:30Z
dc.descriptionA first step in the analysis of the renormalizability of gravity at Large N is carried on. Suitable resummations of planar diagrams give rise to a theory in which there is only a finite number of primitive superficially divergent Feynman diagrams. The mechanism is similar to the the one which makes renormalizable the 3D Gross-Neveu model at large N. Some potential problems in fulfilling the Slavnov-Taylor and the Zinn-Justin equations are also pointed out.
dc.description17 pages, 9 figures. To appear on Phys. Rev. D. Two more references, further technical details and the discussion of the KLT relations at large N have been included
dc.identifierhttps://arxiv.org/abs/hep-th/0608203
dc.identifierhttp://arxiv.org/abs/hep-th/0608203
dc.identifierPhys.Rev. D74 (2006) 064020
dc.identifierdoi:10.1103/PhysRevD.74.064020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/114976
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectMathematical Physics
dc.titleThe UV behavior of Gravity at Large N
dc.typetext

Files

Collections

arXiv