Search results for "Mathematical physics"

showing 10 items of 2687 documents

Operator product expansion coefficients in the exact renormalization group formalism

2020

We study how to compute the operator product expansion coefficients in the exact renormalization group formalism. After discussing possible strategies, we consider some examples explicitly, within the $\epsilon$-expansions, for the Wilson-Fisher fixed points of the real scalar theory in $d=4-\epsilon$ dimensions and the Lee-Yang model in $d=6-\epsilon$ dimensions. Finally we discuss how our formalism may be extended beyond perturbation theory.

High Energy Physics - TheoryPhysics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Scalar (mathematics)FOS: Physical sciencesFixed pointRenormalization group16. Peace & justiceComputer Science::Digital Libraries01 natural sciencesoperator product expansionfield theory in curved spaceFormalism (philosophy of mathematics)Formal aspects of field theoryHigh Energy Physics - Theory (hep-th)fixed point0103 physical sciencesLee-Yang modelOperator product expansionrenormalization group010306 general physicsMathematical physicsperturbation theory
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Bimetric truncations for quantum Einstein gravity and asymptotic safety

2010

In the average action approach to the quantization of gravity the fundamental requirement of "background independence" is met by actually introducing a background metric but leaving it completely arbitrary. The associated Wilsonian renormalization group defines a coarse graining flow on a theory space of functionals which, besides the dynamical metric, depend explicitly on the background metric. All solutions to the truncated flow equations known to date have a trivial background field dependence only, namely via the classical gauge fixing term. In this paper we analyze a number of conceptual issues related to the bimetric character of the gravitational average action and explore a first no…

High Energy Physics - TheoryPhysicsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantGeneral Relativity and Quantum CosmologyRenormalizationGravitationHigh Energy Physics - Theory (hep-th)Quantum gravityBackground independenceCosmological constant problemMathematical physicsGauge fixingAnnals of Physics
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Asymptotically safe Lorentzian gravity.

2011

The gravitational asymptotic safety program strives for a consistent and predictive quantum theory of gravity based on a non-trivial ultraviolet fixed point of the renormalization group (RG) flow. We investigate this scenario by employing a novel functional renormalization group equation which takes the causal structure of space-time into account and connects the RG flows for Euclidean and Lorentzian signature by a Wick-rotation. Within the Einstein-Hilbert approximation, the $\beta$-functions of both signatures exhibit ultraviolet fixed points in agreement with asymptotic safety. Surprisingly, the two fixed points have strikingly similar characteristics, suggesting that Euclidean and Loren…

High Energy Physics - TheoryPhysicsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Euclidean quantum gravityRenormalization groupGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsWick rotationQuantum gravityFunctional renormalization groupUltraviolet fixed pointMathematical physicsPhysical review letters
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Investigating the Ultraviolet Properties of Gravity with a Wilsonian Renormalization Group Equation

2008

We review and extend in several directions recent results on the asymptotic safety approach to quantum gravity. The central issue in this approach is the search of a Fixed Point having suitable properties, and the tool that is used is a type of Wilsonian renormalization group equation. We begin by discussing various cutoff schemes, i.e. ways of implementing the Wilsonian cutoff procedure. We compare the beta functions of the gravitational couplings obtained with different schemes, studying first the contribution of matter fields and then the so-called Einstein-Hilbert truncation, where only the cosmological constant and Newton's constant are retained. In this context we make connection with…

High Energy Physics - TheoryPhysicsAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupFixed pointGeneral Relativity and Quantum CosmologyGravitationHigh Energy Physics - Theory (hep-th)Quantum gravityConstant (mathematics)Scalar curvatureMathematical physics
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Comment on “Topological invariants, instantons, and the chiral anomaly on spaces with torsion”

1999

In Riemann-Cartan spacetimes with torsion only its axial covector piece $A$ couples to massive Dirac fields. Using renormalization group arguments, we show that besides the familiar Riemannian term only the Pontrjagin type four-form $dA\wedge dA$ does arise additionally in the chiral anomaly, but not the Nieh-Yan term $d^\star A$, as has been claimed in a recent paper [PRD 55, 7580 (1997)].

High Energy Physics - TheoryPhysicsChiral anomalyNuclear and High Energy PhysicsInstantonFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupWedge (geometry)General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsLinear formTorsion (algebra)Topological invariantsMathematical physicsPhysical Review D
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Tensor perturbations in a general class of Palatini theories

2015

We study a general class of gravitational theories formulated in the Palatini approach and derive the equations governing the evolution of tensor perturbations. In the absence of torsion, the connection can be solved as the Christoffel symbols of an auxiliary metric which is non-trivially related to the space-time metric. We then consider background solutions corresponding to a perfect fluid and show that the tensor perturbations equations (including anisotropic stresses) for the auxiliary metric around such a background take an Einstein-like form. This facilitates the study in a homogeneous and isotropic cosmological scenario where we explicitly establish the relation between the auxiliary…

High Energy Physics - TheoryPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Space timeTorsion (mechanics)FOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Mathematics::K-Theory and HomologyTensorAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physics
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Polyakov effective action from functional renormalization group equation

2010

We discuss the Polyakov effective action for a minimally coupled scalar field on a two dimensional curved space by considering a non-local covariant truncation of the effective average action. We derive the flow equation for the form factor in $\int\sqrt{g}R c_{k}(\Delta)R$, and we show how the standard result is obtained when we integrate the flow from the ultraviolet to the infrared.

High Energy Physics - TheoryPhysicsFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyAction (physics)High Energy Physics - Theory (hep-th)Flow (mathematics)Functional renormalization groupCovariant transformationCurved spaceEffective actionScalar fieldMathematical physicsAnnals of Physics
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Non-commutative geometry and covariance: From the quantum plane to quantum tensors

1994

Reflection and braid equations for rank two $q$-tensors are derived from the covariance properties of quantum vectors by using the $R$-matrix formalism.

High Energy Physics - TheoryPhysicsFormalism (philosophy of mathematics)High Energy Physics - Theory (hep-th)BraidFOS: Physical sciencesGeneral Physics and AstronomyCovarianceCommutative propertyQuantumMathematical physicsCzechoslovak Journal of Physics
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Wormholes and nonsingular spacetimes in Palatinif(R)gravity

2015

We reconsider the problem of $f(R)$ theories of gravity coupled to Born-Infeld theory of electrodynamics formulated in a Palatini approach, where metric and connection are independent fields. By studying electrovacuum configurations in a static and spherically symmetric space-time, we find solutions which reduce to their Reissner-Nordstr\"om counterparts at large distances but undergo important non-perturbative modifications close to the center. Our new analysis reveals that the point-like singularity is replaced by a finite-size wormhole structure, which provides a geodesically complete and thus nonsingular space-time, despite the existence of curvature divergences at the wormhole throat. …

High Energy Physics - TheoryPhysicsGeodesicSpacetime010308 nuclear & particles physicsCosmic censorship hypothesisFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesSpherically symmetric spacetimeGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsSingularityHigh Energy Physics - Theory (hep-th)Born–Infeld model0103 physical sciencesf(R) gravityWormhole010303 astronomy & astrophysicsMathematical physicsPhysical Review D
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Palatini Approach to Modified Gravity: f(R) Theories and Beyond

2011

We review the recent literature on modified theories of gravity in the Palatini approach. After discussing the motivations that lead to consider alternatives to Einstein's theory and to treat the metric and the connection as independent objects, we review several topics that have been recently studied within this framework. In particular, we provide an in-depth analysis of the cosmic speedup problem, laboratory and solar systems tests, the structure of stellar objects, the Cauchy problem, and bouncing cosmologies. We also discuss the importance of going beyond the f(R) models to capture other phenomenological aspects related with dark matter/energy and quantum gravity.

High Energy Physics - TheoryPhysicsGravity (chemistry)Dark matterStructure (category theory)FOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyConnection (mathematics)High Energy Physics - Phenomenologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Space and Planetary ScienceMetric (mathematics)symbolsInitial value problemQuantum gravityEinsteinMathematical Physics
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