Search results for "Semiclassical gravity"

showing 10 items of 10 documents

Apparent universality of semiclassical gravity in the far field limit

2006

The universality of semiclassical gravity is investigated by considering the behavior of the quantities < ��^2 > and < {T^a}_b >, along with quantum corrections to the effective Newtonian potential in the far field limits of static spherically symmetric objects ranging from stars in the weak field Newtonian limit to black holes. For scalar fields it is shown that when differences occur they all result from the behavior of a single mode with zero frequency and angular momentum and are thus due to a combination of infrared and s-wave effects. An intriguing combination of similarities and differences between the extreme cases of a Schwarzschild black hole and a star in the weak fie…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAngular momentumQuantum field theory in curved spacetimeNewtonian potentialFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Newtonian limitGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsSchwarzschild metricSemiclassical gravityQuantum field theory
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Renormalization group flow of quantum gravity in the Einstein-Hilbert truncation

2002

The exact renormalization group equation for pure quantum gravity is used to derive the non-perturbative $\Fbeta$-functions for the dimensionless Newton constant and cosmological constant on the theory space spanned by the Einstein-Hilbert truncation. The resulting coupled differential equations are evaluated for a sharp cutoff function. The features of these flow equations are compared to those found when using a smooth cutoff. The system of equations with sharp cutoff is then solved numerically, deriving the complete renormalization group flow of the Einstein-Hilbert truncation in $d=4$. The resulting renormalization group trajectories are classified and their physical relevance is discus…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsDensity matrix renormalization groupAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Functional renormalization groupQuantum gravitySemiclassical gravityUltraviolet fixed pointMathematical physicsPhysical Review D
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Pair production due to an electric field in 1+1 dimensions and the validity of the semiclassical approximation

2021

Solutions to the backreaction equation in $1+1$-dimensional semiclassical electrodynamics are obtained and analyzed when considering a time-varying homogeneous electric field initially generated by a classical electric current, coupled to either a quantized scalar field or a quantized spin-$\frac{1}{2}$ field. Particle production by way of the Schwinger effect leads to backreaction effects that modulate the electric field strength. Details of the particle production process are investigated along with the transfer of energy between the electric field and the particles. The validity of the semiclassical approximation is also investigated using a criterion previously implemented for chaotic i…

PhysicsField (physics)010308 nuclear & particles physicsOrder (ring theory)Semiclassical physics01 natural sciencesElectric chargePair production0103 physical sciencesProduction (computer science)Semiclassical gravity010306 general physicsScalar fieldMathematical physicsPhysical Review D
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Is There a C-Function in 4D Quantum Einstein Gravity?

2016

We describe a functional renormalization group-based method to search for ‘C-like’ functions with properties similar to that in 2D conformal field theory. It exploits the mode counting properties of the effective average action and is particularly suited for theories including quantized gravity. The viability of the approach is demonstrated explicitly in a truncation of 4 dimensional Quantum Einstein Gravity, i.e. asymptotically safe metric gravity.

PhysicsGeneral Relativity and Quantum CosmologyClassical mechanicsEntropic gravityHořava–Lifshitz gravityAsymptotic safety in quantum gravityQuantum gravitySpin foamf(R) gravitySemiclassical gravityEuclidean quantum gravityMathematical physics
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The Quantum Scalar Field in Spherically Symmetric Loop Quantum Gravity

2013

We consider the quantization of a spherically symmetric gravitational system coupled to a massless scalar field within the loop quantum gravity framework. Our results rely on the uniform discretizations method developed during the last years. We minimize the associated discrete “master constraint” using a trial state whose gravitational part is peaked around the classical Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyQuantization (physics)Quantum geometryClassical mechanicsSpin foamQuantum gravitySemiclassical gravityLoop quantum gravityScalar fieldLoop quantum cosmology
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Quantum Gravity Effects in the Kerr Spacetime

2010

We analyze the impact of the leading quantum gravity effects on the properties of black holes with nonzero angular momentum by performing a suitable renormalization group improvement of the classical Kerr metric within Quantum Einstein Gravity (QEG). In particular we explore the structure of the horizons, the ergosphere, and the static limit surfaces as well as the phase space avilable for the Penrose process. The positivity properties of the effective vacuum energy momentum tensor are also discussed and the "dressing" of the black hole's mass and angular momentum are investigated by computing the corresponding Komar integrals. The pertinent Smarr formula turns out to retain its classical f…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaKerr metricFOS: Physical sciencesPenrose processBlack holeGeneral Relativity and Quantum CosmologyClassical mechanicsRotating black holeHigh Energy Physics - Theory (hep-th)Total angular momentum quantum numberSemiclassical gravityBlack hole thermodynamics
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RG flows of Quantum Einstein Gravity in the linear-geometric approximation

2014

We construct a novel Wetterich-type functional renormalization group equation for gravity which encodes the gravitational degrees of freedom in terms of gauge-invariant fluctuation fields. Applying a linear-geometric approximation the structure of the new flow equation is considerably simpler than the standard Quantum Einstein Gravity construction since only transverse-traceless and trace part of the metric fluctuations propagate in loops. The geometric flow reproduces the phase-diagram of the Einstein-Hilbert truncation including the non-Gaussian fixed point essential for Asymptotic Safety. Extending the analysis to the polynomial $f(R)$-approximation establishes that this fixed point come…

PhysicsHigh Energy Physics - Theory; High Energy Physics - Theory; General Relativity and Quantum CosmologyHigh Energy Physics - TheoryEntropic gravityGeneral relativityAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Euclidean quantum gravityGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Linearized gravityTheoretical High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGQuantum gravitySemiclassical gravityf(R) gravityAnnals of Physics
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A field theoretic realization of a universal bundle for gravity

1992

Abstract Based upon a local vector supersymmetry algebra, we discuss the general structure of the quantum action for topological gravity theories in arbitrary dimensions. The precise form of the action depends on the particular dimension, and also on the moduli space of interest. We describe the general features by examining a theory of topological gravity in two dimensions, with a moduli space specified by vanishing curvature two-form. It is shown that these topological gravity models together with their observables provide a field theoretic realization of a universal bundle for gravity.

PhysicsNuclear and High Energy PhysicsTopological algebraEntropic gravityHořava–Lifshitz gravityEuclidean quantum gravityHigh Energy Physics::TheoryTheoretical physicsQuantum mechanicsQuantum gravityFiber bundlef(R) gravitySemiclassical gravityGeneral Theoretical Physics
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Focus on quantum Einstein gravity

2012

The gravitational asymptotic safety program summarizes the attempts to construct a consistent and predictive quantum theory of gravity within Wilson's generalized framework of renormalization. Its key ingredient is a non-Gaussian fixed point of the renormalization group flow which controls the behavior of the theory at trans-Planckian energies and renders gravity safe from unphysical divergences. Provided that the fixed point comes with a finite number of ultraviolet-attractive (relevant) directions, this construction gives rise to a consistent quantum field theory which is as predictive as an ordinary, perturbatively renormalizable one. This opens up the exciting possibility of establishin…

PhysicsTheoretical physicsClassical mechanicsEntropic gravityHořava–Lifshitz gravityGeneral relativityAsymptotic safety in quantum gravityGeneral Physics and AstronomyQuantum gravityf(R) gravitySemiclassical gravityUltraviolet fixed pointNew Journal of Physics
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Quantum Einstein Gravity: Towards an Asymptotically Safe Field Theory of Gravity

2007

Physicssymbols.namesakeClassical mechanicsEntropic gravityHořava–Lifshitz gravitysymbolsQuantum gravitySpin foamSemiclassical gravityf(R) gravityHigher-dimensional Einstein gravityEuclidean quantum gravity
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