Search results for "effective action"

showing 10 items of 34 documents

(F, G) -summed form of the QED effective action

2021

We conjecture that the proper-time series expansion of the one-loop effective Lagrangian of quantum electrodynamics can be summed in all terms containing the field-strength invariants $\mathcal{F}=\frac{1}{4}{F}_{\ensuremath{\mu}\ensuremath{\nu}}{F}^{\ensuremath{\mu}\ensuremath{\nu}}(x)$, $\mathcal{G}=\frac{1}{4}{\stackrel{\texttildelow{}}{F}}_{\ensuremath{\mu}\ensuremath{\nu}}{F}^{\ensuremath{\mu}\ensuremath{\nu}}(x)$, including those also possessing derivatives of the electromagnetic field strength. This partial resummation is exactly encapsulated in a factor with the same form as the Heisenberg-Euler Lagrangian density, except that now the electric and magnetic fields can depend arbitrar…

PhysicsConjecture010308 nuclear & particles physics01 natural sciencesMagnetic fieldPair productionElectric field0103 physical sciencesProper timeResummation010306 general physicsSeries expansionEffective actionMathematical physicsPhysical Review D
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Attractive versus repulsive interactions in the Bose-Einstein condensation dynamics of relativistic field theories

2017

We study the impact of attractive self-interactions on the nonequilibrium dynamics of relativistic quantum fields with large occupancies at low momenta. Our primary focus is on Bose-Einstein condensation and nonthermal fixed points in such systems. As a model system we consider O(N)-symmetric scalar field theories. We use classical-statistical real-time simulations, as well as a systematic 1/N expansion of the quantum (2PI) effective action to next-to-leading order. When the mean self-interactions are repulsive, condensation occurs as a consequence of a universal inverse particle cascade to the zero-momentum mode with self-similar scaling behavior. For attractive mean self-interactions the …

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)axionsAnnihilationta114Field (physics)010308 nuclear & particles physicsFOS: Physical sciencesBose-Einstein condensatesCharge (physics)01 natural scienceslaw.inventionHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Q-balllawQuantum electrodynamics0103 physical sciences010306 general physicsScalar fieldQuantumEffective actionBose–Einstein condensateAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Adiabatic regularization with a Yukawa interaction

2017

We extend the adiabatic regularization method for an expanding universe to include the Yukawa interaction between quantized Dirac fermions and a homogeneous background scalar field. We give explicit expressions for the renormalized expectation values of the stress-energy tensor $\langle T_{\mu\nu} \rangle$ and the bilinear $\langle \bar\psi\psi\rangle$ in a spatially flat FLRW spacetime. These are basic ingredients in the semiclassical field equations of fermionic matter in curved spacetime interacting with a background scalar field. The ultraviolet subtracting terms of the adiabatic regularization can be naturally interpreted as coming from appropriate counterterms of the background fields…

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsConformal anomalyHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologySemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Yukawa interaction01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsRegularization (physics)Friedmann–Lemaître–Robertson–Walker metric0103 physical sciencessymbols010306 general physicsAdiabatic processScalar fieldEffective actionMathematical physics
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A note on scaling arguments in the effective average action formalism

2016

The effective average action (EAA) is a scale dependent effective action where a scale $k$ is introduced via an infrared regulator. The $k-$dependence of the EAA is governed by an exact flow equation to which one associates a boundary condition at a scale $\mu$. We show that the $\mu-$dependence of the EAA is controlled by an equation fully analogous to the Callan-Symanzik equation which allows to define scaling quantities straightforwardly. Particular attention is paid to composite operators which are introduced along with new sources. We discuss some simple solutions to the flow equation for composite operators and comment their implications in the case of a local potential approximation.

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsFOS: Physical sciences01 natural sciencesComposite operatorFormalism (philosophy of mathematics)High Energy Physics - Theory (hep-th)0103 physical sciencesBoundary value problem010306 general physicsScalingEffective actionMathematical physics
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Solvable Models for radiating Black Holes and Area-preserving Diffeomorphisms

1995

Solvable theories of 2D dilaton gravity can be obtained from a Liouville theory by suitable field redefinitions. In this paper we propose a new framework to generate 2D dilaton gravity models which can also be exactly solved in the semiclassical approximation. Our approach is based on the recently introduced scheme to quantize massless scalar fields coupled to 2D gravity maintaining invariance under area-preserving diffeomorphisms and Weyl transformations. Starting from the CGHS model with the new effective action we reestablish the full diffeomorphism invariance by means of an adequate family of field redefinitions. The original theory is therefore mapped into a large family of solvable mo…

PhysicsHigh Energy Physics - TheoryAstrofísicaNuclear and High Energy PhysicsGravitacióField (physics)CGHS modelScalar (physics)Semiclassical physicsFOS: Physical sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)symbolsDilatonDiffeomorphismEinsteinEffective actionMathematical physics
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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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Bare Action and Regularized Functional Integral of Asymptotically Safe Quantum Gravity

2009

Investigations of Quantum Einstein Gravity (QEG) based upon the effective average action employ a flow equation which does not contain any ultraviolet (UV) regulator. Its renormalization group trajectories emanating from a non-Gaussian fixed point define asymptotically safe quantum field theories. A priori these theories are, somewhat unusually, given in terms of their effective rather than bare action. In this paper we construct a functional integral representation of these theories. We fix a regularized measure and show that every trajectory of effective average actions, depending on an IR cutoff only, induces an associated trajectory of bare actions which depend on a UV cutoff. Together …

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyRenormalizationClassical mechanicsHigh Energy Physics - Theory (hep-th)Regularization (physics)Path integral formulationQuantum gravityQuantum field theoryEffective action
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Low energy Quantum Gravity from the Effective Average Action

2010

Within the effective average action approach to quantum gravity, we recover the low energy effective action as derived in the effective field theory framework, by studying the flow of possibly non-local form factors that appear in the curvature expansion of the effective average action. We restrict to the one-loop flow where progress can be made with the aid of the non-local heat kernel expansion. We discuss the possible physical implications of the scale dependent low energy effective action through the analysis of the quantum corrections to the Newtonian potential.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Action (physics)General Relativity and Quantum CosmologyRenormalizationClassical mechanicsFlow (mathematics)High Energy Physics - Theory (hep-th)Quantum electrodynamicsEffective field theoryQuantum gravityBeta function (physics)Quantum field theoryEffective action
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Low-energy scattering of extremal black holes by neutral matter

2002

We investigate the decay of a spherically symmetric near-extremal charged black hole, including back-reaction effects, in the near-horizon region. The non-locality of the effective action controlling this process allows and also forces us to introduce a complementary set of boundary conditions which permit to determine the asymptotic late time Hawking flux. The evaporation rate goes down exponentially and admits an infinite series expansion in Planck's constant. At leading order it is proportional to the total mass and the higher order terms involve higher order momenta of the classical stress-tensor. Moreover we use this late time behaviour to go beyond the near-horizon approximation and c…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsScatteringBlack hole information paradoxFluxFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black holeGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Theory (hep-th)Quantum electrodynamicssymbolsFísica nuclearBoundary value problemPlanckSimetria (Física)Constant (mathematics)Effective action
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Conformal and non-conformal symmetries in 2D dilaton gravity

1996

We introduce new extra symmetry transformations for generic 2D dilaton-gravity models. These symmetries are non-conformal but special linear combinations of them turn out to be the extra (conformal) symmetries of the CGHS model and the model with an exponential potential. We show that one of the non-conformal extra symmetries can be converted into a conformal one by means of adequate field redefinitions involving the metric and the derivatives of the dilaton. Finally, by expressing the Polyakov-Liouville effective action in terms of an auxiliary invariant metric, we construct one-loop models which maintain the extra symmetry of the classical action. © 1997 Elsevier Science B.V.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsSigma modelCGHS modelSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Symmetry (physics)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Solvable modelsHomogeneous spaceAstronomiaDilatonInvariant (mathematics)Simetria (Física)Effective actionNon-conformal symmetriesMathematical physics
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