Search results for "Equations"

showing 10 items of 955 documents

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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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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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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Higher genera Catalan numbers and Hirota equations for extended nonlinear Schrödinger hierarchy

2021

We consider the Dubrovin--Frobenius manifold of rank $2$ whose genus expansion at a special point controls the enumeration of a higher genera generalization of the Catalan numbers, or, equivalently, the enumeration of maps on surfaces, ribbon graphs, Grothendieck's dessins d'enfants, strictly monotone Hurwitz numbers, or lattice points in the moduli spaces of curves. Liu, Zhang, and Zhou conjectured that the full partition function of this Dubrovin--Frobenius manifold is a tau-function of the extended nonlinear Schr\"odinger hierarchy, an extension of a particular rational reduction of the Kadomtsev--Petviashvili hierarchy. We prove a version of their conjecture specializing the Givental--M…

High Energy Physics - TheoryPure mathematicsRank (linear algebra)FOS: Physical sciences[MATH] Mathematics [math]01 natural sciencesCatalan numberMathematics::Algebraic Geometry[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]KP hierarchy0103 physical sciences[NLIN] Nonlinear Sciences [physics][NLIN]Nonlinear Sciences [physics][MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]0101 mathematics[MATH]Mathematics [math]Mathematics::Symplectic GeometryMathematical PhysicsMathematicsHirota equationsPartition function (quantum field theory)ConjectureNonlinear Sciences - Exactly Solvable and Integrable SystemsHierarchy (mathematics)010102 general mathematics[MATH.MATH-AG] Mathematics [math]/Algebraic Geometry [math.AG]Statistical and Nonlinear PhysicsMathematical Physics (math-ph)16. Peace & justiceLax equationsManifoldModuli spaceMonotone polygonNonlinear Sciences::Exactly Solvable and Integrable SystemsHigh Energy Physics - Theory (hep-th)010307 mathematical physics[MATH.MATH-AG]Mathematics [math]/Algebraic Geometry [math.AG]Exactly Solvable and Integrable Systems (nlin.SI)Catalan numbersFrobenius manifoldsLetters in Mathematical Physics
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Nonperturbative structure of the ghost-gluon kernel

2019

The ghost-gluon scattering kernel is a special correlation function that is intimately connected with two fundamental vertices of the gauge sector of QCD: the ghost-gluon vertex, which may be obtained from it through suitable contraction, and the three-gluon vertex, whose Slavnov-Taylor identity contains that kernel as one of its main ingredients. In this work we present a detailed nonperturbative study of the five form factors comprising it, using as starting point the `one-loop dressed' approximation of the dynamical equations governing their evolution. The analysis is carried out for arbitrary Euclidean momenta, and makes extensive use of the gluon propagator and the ghost dressing funct…

High Energy Physics - TheoryQuantum chromodynamicsPhysicsHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyFOS: Physical sciencesPropagatorGluonVertex (geometry)High Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeHigh Energy Physics - Theory (hep-th)Lattice (order)Euclidean geometryEquations for a falling bodyTwo-formPhysical Review
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Decomposition of one-loop QCD amplitudes into primitive amplitudes based on shuffle relations

2013

We present the decomposition of QCD partial amplitudes into primitive amplitudes at one-loop level and tree level for arbitrary numbers of quarks and gluons. Our method is based on shuffle relations. This method is purely combinatorial and does not require the inversion of a system of linear equations.

High Energy Physics - TheoryQuarkPhysicsQuantum chromodynamicsNuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciencesSystem of linear equationsGluonHigh Energy Physics - PhenomenologyS-matrix theoryAmplitudeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanicsQuark–gluon plasmaHigh Energy Physics::ExperimentMathematical physics
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Yangian Symmetry for Fishnet Feynman Graphs

2017

Various classes of fishnet Feynman graphs are shown to feature a Yangian symmetry over the conformal algebra. We explicitly discuss scalar graphs in three, four and six spacetime dimensions as well as the inclusion of fermions in four dimensions. The Yangian symmetry results in novel differential equations for these families of largely unsolved Feynman integrals. Notably, the considered fishnet graphs in three and four dimensions dominate the correlation functions and scattering amplitudes in specific double scaling limits of planar, gamma-twisted N=4 super Yang-Mills or ABJM theory. Consequently, the study of fishnet graphs allows us to get deep insights into the integrability of the plana…

High Energy Physics - Theorydimension: 4Feynman graphScalar (mathematics)[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesConformal mapintegrability01 natural sciencesalgebra: conformal[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]symbols.namesake0103 physical sciencesFeynman diagramcorrelation function010306 general physicsABJM modelMathematical PhysicsMathematical physicsPhysicsfield theory: conformalSpacetimeAdS/CFT correspondence010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Mathematical analysisscattering amplitudescalingdifferential equationsMathematical Physics (math-ph)FermionScattering amplitudespace-time: dimension: 6AdS/CFT correspondenceHigh Energy Physics - Theory (hep-th)symmetry: Yangiansupersymmetry: 4symbols[ PHYS.MPHY ] Physics [physics]/Mathematical Physics [math-ph]Yangian
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Unsteadiness and transition to turbulence in woven spacer filled channels for Membrane Distillation

2017

To characterize the performance of Membrane Distillation (MD) modules, channels filled with woven spacers were investigated by Computational Fluid Dynamics (including Direct Numerical Simulations and the use of the SST k-ω turbulence model) and by parallel experiments with Thermochromic Liquid Crystals. The cases considered here regard mutually orthogonal filaments with a spacer pitch to channel height ratio P/H=2, two spacer orientations θ with respect to the main flow (0° and 45°), and bulk Reynolds numbers Re from ∼200 to ∼2000, an interval of great interest in practical MD applications. For both values of θ, CFD predicted steady-state flow for Re up to ∼300, and chaotic flow …

HistoryFlow (psychology)Thermodynamics02 engineering and technologyComputational fluid dynamicsEducationPhysics::Fluid Dynamicssymbols.namesake020401 chemical engineeringLiquid crystal0204 chemical engineeringbusiness.industryTurbulenceChemistryOscillationSpacer-filled channels CFD membrane distillation turbulence RANS DNSReynolds numberMechanics021001 nanoscience & nanotechnologyComputer Science ApplicationsHeat transfersymbols0210 nano-technologyReynolds-averaged Navier–Stokes equationsbusiness
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Generalized Camassa-Holm Equations: Symmetry, Conservation Laws and Regular Pulse and Front Solutions

2021

In this paper, we consider a member of an integrable family of generalized Camassa–Holm (GCH) equations. We make an analysis of the point Lie symmetries of these equations by using the Lie method of infinitesimals. We derive nonclassical symmetries and we find new symmetries via the nonclassical method, which cannot be obtained by Lie symmetry method. We employ the multiplier method to construct conservation laws for this family of GCH equations. Using the conservation laws of the underlying equation, double reduction is also constructed. Finally, we investigate traveling waves of the GCH equations. We derive convergent series solutions both for the homoclinic and heteroclinic orbits of the…

Holm equationsIntegrable systemGeneral MathematicsInfinitesimalNonclassical symmetries01 natural sciencesdouble reduction010305 fluids & plasmas0103 physical sciencesmultiplier methodComputer Science (miscellaneous)QA1-939Generalized Camassa–Holm equationsHomoclinic orbit010306 general physicsEngineering (miscellaneous)Settore MAT/07 - Fisica MatematicaConvergent seriesmulti-infinite series solutionsMathematicsMathematical physicsConservation lawsnonclassical symmetriesConservation lawHomoclinic and heteroclinic orbitsMulti-infinite series solutionsDouble reductionSymmetry (physics)Pulse (physics)generalized Camassa&#8211Mathematics::LogicMultiplier methodHomogeneous spaceconservation lawshomoclinic and heteroclinic orbitsMathematics
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