Search results for "Functional renormalization group"

showing 10 items of 25 documents

Why the Cosmological Constant Seems to Hardly Care About Quantum Vacuum Fluctuations: Surprises From Background Independent Coarse Graining

2020

International audience; Background Independence is a sine qua non for every satisfactory theory of Quantum Gravity. In particular if one tries to establish a corresponding notion of Wilsonian renormalization, or coarse graining, it presents a major conceptual and technical difficulty usually. In this paper we adopt the approach of the gravitational Effective Average Action and demonstrate that generically coarse graining in Quantum Gravity and in standard field theories on a non-dynamical spacetime are profoundly different. By means of a concrete example, which in connection with the cosmological constant problem is also interesting in its own right, we show that the surprising and sometime…

Materials Science (miscellaneous)Background independent quantum gravityBiophysicsAsymptotic safety in quantum gravityGeneral Physics and AstronomyCosmological constantnonperturbativeasymptotic safety01 natural sciencesrenormalizationGravitationRenormalizationTheoretical physicsVacuum energyFunctional renormalisation group0103 physical sciencesultravioletBackground independencePhysical and Theoretical Chemistry010306 general physicsMathematical PhysicsPhysicsenergy: highcosmological constantbackgroundfunctional renormalization grouplcsh:QC1-999fluctuation: vacuumspace-timegravitationquantum gravity[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Quantum gravityrenormalisation grouprenormalization grouplcsh:PhysicsCosmological constant problem
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The Functional Renormalization Group

2018

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PhysicsCambridge Monographs on Mathematical PhysicsTheoretical High Energy PhysicsFunctional renormalization groupHigh Energy PhysicsMathematical physics
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Complex-mass renormalization in chiral effective field theory

2009

We consider a low-energy effective field theory of vector mesons and Goldstone bosons using the complex-mass renormalization. As an application we calculate the mass and the width of the $\rho$ meson.

PhysicsCondensed Matter::Quantum GasesRenormalizationParticle physicsNuclear and High Energy PhysicsMesonHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesRenormalizationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Effective filed theoryGoldstone bosonEffective field theoryFunctional renormalization groupHigh Energy Physics::ExperimentVector mesonsCritical dimension
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Bimetric Renormalization Group Flows in Quantum Einstein Gravity

2011

The formulation of an exact functional renormalization group equation for Quantum Einstein Gravity necessitates that the underlying effective average action depends on two metrics, a dynamical metric giving the vacuum expectation value of the quantum field, and a background metric supplying the coarse graining scale. The central requirement of "background independence" is met by leaving the background metric completely arbitrary. This bimetric structure entails that the effective average action may contain three classes of interactions: those built from the dynamical metric only, terms which are purely background, and those involving a mixture of both metrics. This work initiates the first …

PhysicsHigh Energy Physics - TheoryBackground field methodAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyGravitationTheoretical physicsHigh Energy Physics - Theory (hep-th)Functional renormalization groupQuantum gravityBackground independenceEffective action
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Functional and local renormalization groups

2015

We discuss the relation between functional renormalization group (FRG) and local renormalization group (LRG), focussing on the two dimensional case as an example. We show that away from criticality the Wess-Zumino action is described by a derivative expansion with coefficients naturally related to RG quantities. We then demonstrate that the Weyl consistency conditions derived in the LRG approach are equivalent to the RG equation for the $c$-function available in the FRG scheme. This allows us to give an explicit FRG representation of the Zamolodchikov-Osborn metric, which in principle can be used for computations.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsFOS: Physical sciencesFunction (mathematics)General Relativity and Quantum Cosmology (gr-qc)Renormalization groupCondensed Matter::Disordered Systems and Neural NetworksAction (physics)General Relativity and Quantum CosmologyRenormalizationHigh Energy Physics - Theory (hep-th)Scheme (mathematics)Theoretical High Energy PhysicsMetric (mathematics)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFunctional renormalization groupRepresentation (mathematics)Mathematical physics
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Ultraviolet Fixed Point and Generalized Flow Equation of Quantum Gravity

2001

A new exact renormalization group equation for the effective average action of Euclidean quantum gravity is constructed. It is formulated in terms of the component fields appearing in the transverse-traceless decomposition of the metric. It facilitates both the construction of an appropriate infrared cutoff and the projection of the renormalization group flow onto a large class of truncated parameter spaces. The Einstein-Hilbert truncation is investigated in detail and the fixed point structure of the resulting flow is analyzed. Both a Gaussian and a non-Gaussian fixed point are found. If the non-Gaussian fixed point is present in the exact theory, quantum Einstein gravity is likely to be r…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsInfrared fixed pointAsymptotic safety in quantum gravityGravitonFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Euclidean quantum gravityRenormalization groupGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum gravityFunctional renormalization groupUltraviolet fixed pointMathematical physics
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En route to Background Independence: Broken split-symmetry, and how to restore it with bi-metric average actions

2014

The most momentous requirement a quantum theory of gravity must satisfy is Background Independence, necessitating in particular an ab initio derivation of the arena all non-gravitational physics takes place in, namely spacetime. Using the background field technique, this requirement translates into the condition of an unbroken split-symmetry connecting the (quantized) metric fluctuations to the (classical) background metric. If the regularization scheme used violates split-symmetry during the quantization process it is mandatory to restore it in the end at the level of observable physics. In this paper we present a detailed investigation of split-symmetry breaking and restoration within the…

PhysicsHigh Energy Physics - TheorySpacetimeAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyQuantization (physics)Theoretical physicsHigh Energy Physics - Theory (hep-th)Regularization (physics)Quantum gravityFunctional renormalization groupBackground independence
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Einstein-Cartan gravity, Asymptotic Safety, and the running Immirzi parameter

2013

In this paper we analyze the functional renormalization group flow of quantum gravity on the Einstein-Cartan theory space. The latter consists of all action functionals depending on the spin connection and the vielbein field (co-frame) which are invariant under both spacetime diffeomorphisms and local frame rotations. In the first part of the paper we develop a general methodology and corresponding calculational tools which can be used to analyze the flow equation for the pertinent effective average action for any truncation of this theory space. In the second part we apply it to a specific three-dimensional truncated theory space which is parametrized by Newton's constant, the cosmological…

PhysicsHigh Energy Physics - TheorySpacetimeImmirzi parameterAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantRenormalization groupGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum gravityFunctional renormalization groupSpin connection
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Non-perturbative renormalization of lattice operators in coordinate space

2004

We present the first numerical implementation of a non-perturbative renormalization method for lattice operators, based on the study of correlation functions in coordinate space at short Euclidean distance. The method is applied to compute the renormalization constants of bilinear quark operators for the non-perturbative O(a)-improved Wilson action in the quenched approximation. The matching with perturbative schemes, such as MS-bar, is computed at the next-to-leading order in continuum perturbation theory. A feasibility study of this technique with Neuberger fermions is also presented.

PhysicsNuclear and High Energy PhysicsHigh Energy Physics::Latticefield theory gauge theory lattice renormalizationHigh Energy Physics - Lattice (hep-lat)FísicaFOS: Physical sciencesQuenched approximationFIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIRenormalizationEuclidean distanceHigh Energy Physics - LatticeOperator (computer programming)Quantum mechanicsFunctional renormalization groupPerturbation theory (quantum mechanics)Coordinate spaceNon-perturbativeMathematical physics
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Renormalization of relativistic baryon chiral perturbation theory and power counting

2003

We discuss a renormalization scheme for relativistic baryon chiral perturbation theory which provides a simple and consistent power counting for renormalized diagrams. The method involves finite subtractions of dimensionally regularized diagrams beyond the standard $\bar{\rm MS}$ scheme of chiral perturbation theory to remove contributions violating the power counting. This is achieved by a suitable renormalization of the parameters of the most general effective Lagrangian. In addition to simplicity our method has the benefit that it can be easily applied to multiloop diagrams. As an application we discuss the mass and the scalar form factor of the nucleon and compare the results with the e…

PhysicsNuclear and High Energy PhysicsParticle physicsChiral perturbation theoryNuclear Theory010308 nuclear & particles physicsHigh Energy Physics::LatticeFOS: Physical sciences01 natural sciencesBaryonRenormalizationNuclear Theory (nucl-th)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Regularization (physics)0103 physical sciencesEffective lagrangianFunctional renormalization group010306 general physicsNucleonNuclear theoryMathematical physics
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