Search results for "RENORMALIZATION"

showing 10 items of 470 documents

R2phase diagram of quantum Einstein gravity and its spectral dimension

2012

Within the gravitational asymptotic safety program, the renormalization group (RG) flow of the ${R}^{2}$ truncation in three and four spacetime dimensions is analyzed in detail. In particular, we construct RG trajectories which emanate from the non-Gaussian UV fixed point and possess long classical regimes where the effective average action is well approximated by the classical Einstein-Hilbert action. As an application we study the spectral dimension of the effective quantum Einstein gravity spacetimes resulting from these trajectories, establishing that the picture of a multifractal spacetime is robust under the extension of the truncated theory space. We demonstrate that regimes of const…

PhysicsGravitationGeneral Relativity and Quantum CosmologyNuclear and High Energy PhysicsSpacetimeGeneral relativityQuantum mechanicsAsymptotic safety in quantum gravityQuantum gravityFixed pointRenormalization groupUltraviolet fixed pointMathematical physicsPhysical Review D
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Quantum gravity with torsion and non-metricity

2015

We study the renormalization of theories of gravity with an arbitrary (torsionful and non-metric) connection. The class of actions we consider is of the Palatini type, including the most general terms with up to two derivatives of the metric, but no derivatives of the connection. It contains 19 independent parameters. We calculate the one loop beta functions of these parameters and find their fixed points. The Holst subspace is discussed in some detail and found not to be stable under renormalization. Some possible implications for ultraviolet and infrared gravity are discussed.

PhysicsGravity (chemistry)Physics and Astronomy (miscellaneous)torsion and non-metricityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointGeneral Relativity and Quantum CosmologyConnection (mathematics)Settore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciRenormalizationquantum gravity; renormalization group; torsion and non-metricityquantum gravityMetric (mathematics)Torsion (algebra)Quantum gravityrenormalization groupSubspace topologyMathematical physics
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Renormalisation group study of Anderson localisation in two dimensions: effect of second-order terms

1981

The localisation of electrons moving in a random potential is studied in two dimensions using the real space renormalisation group method of Domany and Sarker. The effects of the cell size and of the second-order terms in the perturbation expansion are examined. While the method is not particularly sensitive to the cell size, its results depend crucially on the truncation of the perturbation series.

PhysicsGroup studyCondensed matter physicsGeneral EngineeringGeneral Physics and AstronomyPerturbation (astronomy)Elementary particleElectronFermionCondensed Matter PhysicsPotential energyRenormalizationStatistical physicsLeptonJournal of Physics C: Solid State Physics
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Relativistic Magnetohydrodynamics: Renormalized eigenvectors and full wave decomposition Riemann solver

2010

We obtain renormalized sets of right and left eigenvectors of the flux vector Jacobians of the relativistic MHD equations, which are regular and span a complete basis in any physical state including degenerate ones. The renormalization procedure relies on the characterization of the degeneracy types in terms of the normal and tangential components of the magnetic field to the wavefront in the fluid rest frame. Proper expressions of the renormalized eigenvectors in conserved variables are obtained through the corresponding matrix transformations. Our work completes previous analysis that present different sets of right eigenvectors for non-degenerate and degenerate states, and can be seen as…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Degenerate energy levelsFOS: Physical sciencesAstronomy and AstrophysicsSolverRest frameRiemann solverRenormalizationsymbols.namesakeTransformation matrixSpace and Planetary SciencesymbolsApplied mathematicsDegeneracy (mathematics)Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaInstrumentation and Methods for Astrophysics (astro-ph.IM)Eigenvalues and eigenvectorsAstrophysics - Cosmology and Nongalactic Astrophysics
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Products of current operators in the exact renormalization group formalism

2020

Given a Wilson action invariant under global chiral transformations, we can construct current composite operators in terms of the Wilson action. The short distance singularities in the multiple products of the current operators are taken care of by the exact renormalization group. The Ward-Takahashi identity is compatible with the finite momentum cutoff of the Wilson action. The exact renormalization group and the Ward-Takahashi identity together determine the products. As a concrete example, we study the Gaussian fixed-point Wilson action of the chiral fermions to construct the products of current operators.

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsDifferential equationGaussianHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesRenormalization group01 natural sciencesShort distanceComposite operatorFormalism (philosophy of mathematics)symbols.namesakeHigh Energy Physics - Theory (hep-th)0103 physical sciencessymbolsCutoffGravitational singularity010306 general physicsMathematical physicsProgress of Theoretical and Experimental Physics
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Role of gravity in the pair creation induced by electric fields

2018

We analyze the pair production induced by homogenous, time-dependent electric fields in an expanding space-time background. We point out that, in obtaining the semiclassical Maxwell equations, two distinct notions of adiabatic renormalization are possible. In Minkowski space the two recipes turn out to be equivalent. However, in the presence of gravity only the recipe requiring an adiabatic hierarchy between the gravitational and the gauge field is consistent with the conservation of the energy-momentum tensor.

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGravitationsymbols.namesakeClassical mechanicsMaxwell's equationsHigh Energy Physics - Theory (hep-th)0103 physical sciencesMinkowski spacesymbolsTensorGauge theory010306 general physicsAdiabatic process
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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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Local BRST cohomology in gauge theories

2000

The general solution of the anomaly consistency condition (Wess-Zumino equation) has been found recently for Yang-Mills gauge theory. The general form of the counterterms arising in the renormalization of gauge invariant operators (Kluberg-Stern and Zuber conjecture) and in gauge theories of the Yang-Mills type with non power counting renormalizable couplings has also been worked out in any number of spacetime dimensions. This Physics Report is devoted to reviewing in a self-contained manner these results and their proofs. This involves computing cohomology groups of the differential introduced by Becchi, Rouet, Stora and Tyutin, with the sources of the BRST variations of the fields ("antif…

PhysicsHigh Energy Physics - TheoryConservation lawSpacetimeHigh Energy Physics::LatticeGeneral Physics and AstronomyFOS: Physical sciencesInvariant (physics)CohomologyBRST quantizationRenormalizationTheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Gauge theoryAlgebraic number
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Cosmological Perturbations in Renormalization Group Derived Cosmologies

2002

A linear cosmological perturbation theory of an almost homogeneous and isotropic perfect fluid Universe with dynamically evolving Newton constant $G$ and cosmological constant $\Lambda$ is presented. A gauge-invariant formalism is developed by means of the covariant approach, and the acoustic propagation equations governing the evolution of the comoving fractional spatial gradients of the matter density, $G$, and $\Lambda$ are thus obtained. Explicit solutions are discussed in cosmologies where both $G$ and $\Lambda$ vary according to renormalization group equations in the vicinity of a fixed point.

PhysicsHigh Energy Physics - TheoryIsotropyAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsPerfect fluidCosmological constantAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsFixed pointRenormalization groupAstrophysicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceHomogeneousCosmological perturbation theoryCovariant transformationMathematical PhysicsMathematical physics
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Finite Entanglement Entropy in Asymptotically Safe Quantum Gravity

2018

Entanglement entropies calculated in the framework of quantum field theory on classical, flat or curved, spacetimes are known to show an intriguing area law in four dimensions, but they are also notorious for their quadratic ultraviolet divergences. In this paper we demonstrate that the analogous entanglement entropies when computed within the Asymptotic Safety approach to background independent quantum gravity are perfectly free from such divergences. We argue that the divergences are an artifact due to the over-idealization of a rigid, classical spacetime geometry which is insensitive to the quantum dynamics.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsQuantum dynamicsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Quantum entanglementRenormalization group01 natural sciencesGeneral Relativity and Quantum CosmologySpacetime geometryTheoretical physicsQuadratic equationHigh Energy Physics - Theory (hep-th)0103 physical sciencesModels of Quantum Gravitylcsh:QC770-798Quantum gravityRenormalization Grouplcsh:Nuclear and particle physics. Atomic energy. RadioactivityQuantum field theory010306 general physics
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