Asymptotic safe nonassociative quantum gravity with star R-flux products, Goroff-Sagnotti counter-terms, and geometric flows
S. Vacaru

TL;DR
This paper demonstrates that nonassociative modifications of general relativity, involving R-flux deformations, can be formulated as viable quantum gravity theories through generalized asymptotic safety and geometric flow techniques.
Contribution
It introduces a new nonholonomic functional renormalization approach for nonassociative quantum gravity with R-flux deformations, establishing their consistency and viability.
Findings
Nonassociative gravity theories can be well-defined as classical and quantum models.
Generalized G. Perelman thermodynamic variables are computed for nonassociative flows.
Effective models with off-diagonal solutions support asymptotic safety in nonassociative QG.
Abstract
Nonassociative modifications of general relativity, GR, defined by star products with R-flux deformations in string gravity consist of an important subclass of modified gravity theories, MGTs. A longstanding criticism for elaborating quantum gravity, QG, argue that the asymptotic safety does not survive once certain perturbative terms (in general, nonassociative and noncommutative) are included in the projection space. The goal of this work is to prove that a generalized asymptotic safety scenario allows us to formulate physically viable nonassociative QG theories using effective models defined by generic off-diagonal solutions and nonlinear symmetries in nonassociative geometric flow and gravity theories. We elaborate on a new nonholonomic functional renormalization techniques with parametric renormalization group, RG, flow equations for effective actions supplemented by certain…
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