Search results for "equation"

showing 10 items of 4219 documents

Gluon mass generation in the PT-BFM scheme

2006

In this article we study the general structure and special properties of the Schwinger-Dyson equation for the gluon propagator constructed with the pinch technique, together with the question of how to obtain infrared finite solutions, associated with the generation of an effective gluon mass. Exploiting the known all-order correspondence between the pinch technique and the background field method, we demonstrate that, contrary to the standard formulation, the non-perturbative gluon self-energy is transverse order-by-order in the dressed loop expansion, and separately for gluonic and ghost contributions. We next present a comprehensive review of several subtle issues relevant to the search …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsBackground field methodLorentz transformationHigh Energy Physics::LatticeMass generationHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyPropagatorFOS: Physical sciencesFísicaRenormalization groupIntegral equationMassless particleHigh Energy Physics - Phenomenologysymbols.namesakeTheoretical physicsDimensional regularizationHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)symbols
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Limits on the parameters of the equation of state for interacting dark energy

2010

Under the assumption that cold dark matter and dark energy interact with each other through a small coupling term, $Q$, we constrain the parameter space of the equation of state $w$ of those dark energy fields whose variation of the field since last scattering do not exceed Planck's mass. We use three parameterizations of $w$ and two different expressions for $Q$. Our work extends previous ones.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsEquation of stateCosmology and Nongalactic Astrophysics (astro-ph.CO)Hot dark matterScalar field dark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyThermodynamics of the universeHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum electrodynamicsMixed dark matterWarm dark matterDark energyLight dark matterDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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Cosmological Horizon Modes and Linear Response in de Sitter Spacetime

2009

Linearized fluctuations of quantized matter fields and the spacetime geometry around de Sitter space are considered in the case that the matter fields are conformally invariant. Taking the unperturbed state of the matter to be the de Sitter invariant Bunch-Davies state, the linear variation of the stress tensor about its self-consistent mean value serves as a source for fluctuations in the geometry through the semiclassical Einstein equations. This linear response framework is used to investigate both the importance of quantum backreaction and the validity of the semiclassical approximation in cosmology. The full variation of the stress tensor delta bi contains two kinds of terms: (1) those…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetimeCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsCauchy stress tensorDe Sitter spaceSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyAuxiliary fieldGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum cosmologyQuantum mechanics0103 physical sciencesEinstein field equations010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physics
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Noncommutative space and the low-energy physics of quasicrystals

2008

We prove that the effective low-energy, nonlinear Schroedinger equation for a particle in the presence of a quasiperiodic potential is the potential-free, nonlinear Schroedinger equation on noncommutative space. Thus quasiperiodicity of the potential can be traded for space noncommutativity when describing the envelope wave of the initial quasiperiodic wave.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsQuasicrystalFOS: Physical sciencesAstronomy and AstrophysicsMathematical Physics (math-ph)Space (mathematics)Noncommutative geometryAtomic and Molecular Physics and OpticsNonlinear Sciences::Chaotic DynamicsQuasiperiodicitysymbols.namesakeLow energyHigh Energy Physics - Theory (hep-th)Quasiperiodic functionsymbolsNonlinear Schrödinger equationMathematical PhysicsMathematical physicsEnvelope (waves)
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Free field realization of cylindrically symmetric Einstein gravity

1998

Cylindrically reduced Einstein gravity can be regarded as an $SL(2,R)/SO(2)$ sigma model coupled to 2D dilaton gravity. By using the corresponding 2D diffeomorphism algebra of constraints and the asymptotic behaviour of the Ernst equation we show that the theory can be mapped by a canonical transformation into a set of free fields with a Minkowskian target space. We briefly discuss the quantization in terms of these free-field variables, which is considerably simpler than in the other approaches.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSigma modelFOS: Physical sciencesCanonical transformationGeneral Relativity and Quantum Cosmology (gr-qc)Free fieldGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeQuantization (physics)High Energy Physics - Theory (hep-th)symbolsFísica nuclearDilatonNernst equationDiffeomorphismEinsteinMathematical physicsPhysics Letters B
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Lorentz harmonics and superfield action. D=10, N=1 superstring

2000

We propose a new version of the superfield action for a closed D=10, N=1 superstring where the Lorentz harmonics are used as auxiliary superfields. The incorporation of Lorentz harmonics into the superfield action makes possible to obtain superfield constraints of the induced worldsheet supergravity as equations of motion. Moreover, it becomes evident that a so-called 'Wess-Zumino part' of the superfield action is basically a Lagrangian form of the generalized action principle. We propose to use the second Noether theorem to handle the essential terms in the transformation lows of hidden gauge symmetries, which remove dynamical degrees of freedom from the Lagrange multiplier superfield.

High Energy Physics - TheoryPhysicsPhysics and Astronomy (miscellaneous)WorldsheetLorentz transformationSupergravityHigh Energy Physics::PhenomenologySuperstring theoryEquations of motionFOS: Physical sciencesSuperspaceAction (physics)symbols.namesakeHigh Energy Physics::TheoryNonlinear Sciences::Exactly Solvable and Integrable SystemsHigh Energy Physics - Theory (hep-th)symbolsNoether's theoremMathematical physics
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General invertible transformation and physical degrees of freedom

2017

An invertible field transformation is such that the old field variables correspond one-to-one to the new variables. As such, one may think that two systems that are related by an invertible transformation are physically equivalent. However, if the transformation depends on field derivatives, the equivalence between the two systems is nontrivial due to the appearance of higher derivative terms in the equations of motion. To address this problem, we prove the following theorem on the relation between an invertible transformation and Euler-Lagrange equations: If the field transformation is invertible, then any solution of the original set of Euler-Lagrange equations is mapped to a solution of …

High Energy Physics - TheoryPhysicsPure mathematicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquations of motionMaterial derivativeClassical Physics (physics.class-ph)FOS: Physical sciencesPhysics - Classical PhysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTensor fieldlaw.inventionField transformationInvertible matrixHigh Energy Physics - Theory (hep-th)law0103 physical sciencesEquivalence (formal languages)010306 general physicsField equationScalar fieldAstrophysics - Cosmology and Nongalactic Astrophysics
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The Bethe ansatz and the Tzitzéica–Bullough–Dodd equation

2012

The theory of classically integrable nonlinear wave equations, and the Bethe Ansatz systems describing massive quantum field theories defined on an infinite cylinder, are related by an important mathematical correspondence that still lacks a satisfactory physical interpretation. In this paper we shall describe this link for the case of the classical and quantum versions of the (Tzitz\'eica-)Bullough-Dodd model.

High Energy Physics - TheoryPhysicsQuantum PhysicsQuantum sigma modelsIntegrable system010308 nuclear & particles physicsGeneral MathematicsGeneral EngineeringGeneral Physics and AstronomyODE/IM correspondenceQuantum sigma models ODE/IM correspondence01 natural sciencesBethe ansatzNonlinear Sciences::Exactly Solvable and Integrable SystemsNonlinear wave equation0103 physical sciencesCylinderQuantum field theory010306 general physicsMathematical PhysicsMathematical physicsPhilosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences
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Gluon mass scale through nonlinearities and vertex interplay

2019

We present a novel analysis of the gluon gap equation, where its full nonlinear structure is duly taken into account. In particular, while in previous treatments the linearization of this homogeneous integral equation introduced an indeterminacy in the scale of the corresponding mass, the current approach determines it uniquely, once the value of the gauge coupling at a given renormalization point is used as input. A crucial ingredient for this construction is the "kinetic term" of the gluon propagator, whose form is not obtained from the complicated equation governing its evolution, but is rather approximated by suitable initial {\it Ans\"atze}, which are subsequently improved by means of …

High Energy Physics - TheoryPhysicsQuark010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyHigh Energy Physics - Lattice (hep-lat)PropagatorFOS: Physical sciences01 natural sciencesIntegral equationVertex (geometry)GluonRenormalizationHigh Energy Physics - PhenomenologyHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)LinearizationLattice (order)0103 physical sciences010306 general physicsMathematical physics
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Generalized Slow Roll in the Unified Effective Field Theory of Inflation

2017

We provide a compact and unified treatment of power spectrum observables for the effective field theory (EFT) of inflation with the complete set of operators that lead to second-order equations of motion in metric perturbations in both space and time derivatives, including Horndeski and GLPV theories. We relate the EFT operators in ADM form to the four additional free functions of time in the scalar and tensor equations. Using the generalized slow roll formalism, we show that each power spectrum can be described by an integral over a single source that is a function of its respective sound horizon. With this correspondence, existing model independent constraints on the source function can b…

High Energy Physics - TheoryPhysicsSource functionCosmology and Nongalactic Astrophysics (astro-ph.CO)Slow rollSpacetime010308 nuclear & particles physicsScalar (mathematics)Spectral densityEquations of motionFOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesEffective field theory010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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