Search results for "Equations"

showing 10 items of 955 documents

Cosmological Constant and Local Gravity

2010

We discuss the linearization of Einstein equations in the presence of a cosmological constant, by expanding the solution for the metric around a flat Minkowski space-time. We demonstrate that one can find consistent solutions to the linearized set of equations for the metric perturbations, in the Lorentz gauge, which are not spherically symmetric, but they rather exhibit a cylindrical symmetry. We find that the components of the gravitational field satisfying the appropriate Poisson equations have the property of ensuring that a scalar potential can be constructed, in which both contributions, from ordinary matter and Lambda > 0, are attractive. In addition, there is a novel tensor potentia…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)De Sitter spaceFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyDe Sitter universeLinearized gravity0103 physical sciencesMinkowski spaceSchwarzschild metric010303 astronomy & astrophysicsMathematical physicsPhysicsInhomogeneous cosmology010308 nuclear & particles physicsGeneral Relativity and CosmologyFísicaClassical mechanicsLorenz gauge conditionHigh Energy Physics - Theory (hep-th)Einstein field equationsAstrophysics - Cosmology and Nongalactic Astrophysics
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High-energy evolution to three loops

2018

The Balitsky-Kovchegov equation describes the high-energy growth of gauge theory scattering amplitudes as well as nonlinear saturation effects which stop it. We obtain the three-loop corrections to this equation in planar $\mathcal{N}=4$ super Yang-Mills theory. Our method exploits a recently established equivalence with the physics of soft wide-angle radiation, so-called non-global logarithms, and thus yields at the same time the three-loop evolution equation for non-global logarithms. As a by-product of our analysis, we develop a Lorentz-covariant method to subtract infrared and collinear divergences in cross-section calculations in the planar limit. We compare our result in the linear re…

High Energy Physics - TheoryNuclear and High Energy PhysicsDifferential equationFOS: Physical sciencesYang–Mills theory01 natural sciences114 Physical sciencesperturbative QCDSupersymmetric Gauge TheoryPomeronHARMONIC POLYLOGARITHMSHigh Energy Physics - Phenomenology (hep-ph)supersymmetriaPerturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityGauge theoryLimit (mathematics)Scattering Amplitudes010306 general physicsQCD AMPLITUDESsupersymmetric gauge theoryMathematical physicsPhysicsPOMERONta114010308 nuclear & particles physicsMASS SINGULARITIESPerturbative QCDDIFFERENTIAL-EQUATIONSscattering amplitudesScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Supersymmetric gauge theoryresummationYANG-MILLS THEORYlcsh:QC770-798ResummationkvanttikenttäteoriaTO-LEADING ORDERGAUGE-THEORYAPPROXIMATIONJournal of High Energy Physics
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Transplanckian inflation as gravity echoes

2015

In this work, we show that, in the presence of non-minimal coupling to gravity, it is possible to generate sizeable tensor modes in single-field models without transplanckian field values. These transplanckian field values apparently needed in Einstein gravity to accommodate the experimental results may only be due to our insistence of imposing a minimal coupling of the inflaton field to gravity in a model with non-minimal couplings. We present three simple single-field models that prove that it is possible accommodate a large tensor-to-scalar ratio without requiring transplanckian field values within the slow-roll regime.

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)FOS: Physical sciences01 natural sciencesGravitationTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTensor010306 general physicsMinimal couplingPhysicsInflation (cosmology)010308 nuclear & particles physicsFísicaInflatonlcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Einstein field equationslcsh:PhysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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On the zero crossing of the three-gluon vertex

2016

We report on new results on the infrared behaviour of the three-gluon vertex in quenched Quantum Chormodynamics, obtained from large-volume lattice simulations. The main focus of our study is the appearance of the characteristic infrared feature known as 'zero crossing', the origin of which is intimately connected with the nonperturbative masslessness of the Faddeev-Popov ghost. The appearance of this effect is clearly visible in one of the two kinematic configurations analyzed, and its theoretical origin is discussed in the framework of Schwinger-Dyson equations. The effective coupling in the momentum subtraction scheme that corresponds to the three-gluon vertex is constructed, revealing t…

High Energy Physics - TheoryNuclear and High Energy PhysicsLattice simulationsInfraredHigh Energy Physics::LatticeFOS: Physical sciencesThree-gluon vertexKinematicsnonperturbative01 natural sciencesSchwinger–Dyson equations[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]High Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeQuantum mechanicsLattice (order)0103 physical sciencesddc:530Exact locationquantum chromodynamics: quenching010306 general physicsMathematical physicslatticeQuantum chromodynamicsPhysicsZero crossing010308 nuclear & particles physics[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat][PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]High Energy Physics::PhenomenologyHigh Energy Physics - Lattice (hep-lat)[ PHYS.HLAT ] Physics [physics]/High Energy Physics - Lattice [hep-lat]gluon: vertexcrossingZero crossingghostlcsh:QC1-999GluonDyson-Schwinger equationHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]infrared[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:Physics
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Infrared facets of the three-gluon vertex

2021

We present novel lattice results for the form factors of the quenched three-gluon vertex of QCD, in two special kinematic configurations that depend on a single momentum scale. We consider three form factors, two associated with a classical tensor structure and one without tree-level counterpart, exhibiting markedly different infrared behaviors. Specifically, while the former display the typical suppression driven by a negative logarithmic singularity at the origin, the latter saturates at a small negative constant. These exceptional features are analyzed within the Schwinger-Dyson framework, with the aid of special relations obtained from the Slavnov-Taylor identities of the theory. The em…

High Energy Physics - TheoryNuclear and High Energy PhysicsQC1-999High Energy Physics::LatticeFOS: Physical sciencesThree-gluon vertexLattice QCD01 natural sciencesMomentumTheoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)SingularitySchwinger-Dyson equations0103 physical sciencesTensor010306 general physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsPhysicsHigh Energy Physics - Lattice (hep-lat)Lattice QCDQCDHigh Energy Physics - PhenomenologyLattice (module)High Energy Physics - Theory (hep-th)Vertex (curve)Constant (mathematics)Physics Letters B
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Finite size spectrum of SU(N) principal chiral field from discrete Hirota dynamics

2016

Using recently proposed method of discrete Hirota dynamics for integrable (1+1)D quantum field theories on a finite space circle of length L, we derive and test numerically a finite system of nonlinear integral equations for the exact spectrum of energies of SU(N)xSU(N) principal chiral field model as functions of m L, where m is the mass scale. We propose a determinant solution of the underlying Y-system, or Hirota equation, in terms of determinants (Wronskians) of NxN matrices parameterized by N-1 functions of the spectral parameter, with the known analytical properties at finite L. Although the method works in principle for any state, the explicit equations are written for states in the …

High Energy Physics - TheoryNuclear and High Energy PhysicsSigma modelField (physics)FOS: Physical sciences2 dimensionsrepresentation-theory01 natural sciencesexcited-state energiesnonlinear integral-equationsQuantum mechanics0103 physical sciencesBound statelcsh:Nuclear and particle physics. Atomic energy. Radioactivityvolume dependenceQuantum field theory010306 general physicsS-matrixMathematical physicsPhysics[PHYS]Physics [physics][ PHYS ] Physics [physics]010308 nuclear & particles physicsWronskiano(n) sigma-modeln phase-transitionState (functional analysis)goldstone bosonsAdS/CFT correspondenceHigh Energy Physics - Theory (hep-th)lcsh:QC770-798tba equations
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Pinch Technique: Theory and Applications

2009

We review the theoretical foundations and the most important physical applications of the Pinch Technique (PT). This general method allows the construction of off-shell Green’s functions in non-Abelian gauge theories that are independent of the gauge-fixing parameter and satisfy ghost-free Ward identities. We first present the diagrammatic formulation of the technique in QCD, deriving, at one loop, the gauge independent gluon self-energy, quark–gluon vertex, and three-gluon vertex, together with their Abelian Ward identities. The generalization of the PT to theories with spontaneous symmetry breaking is carried out in detail, and the profound connection with the optical theorem and the disp…

High Energy Physics - TheoryParticle physicsSpontaneous symmetry breakingGluonsHigh Energy Physics::LatticeFOS: Physical sciencesGeneral Physics and AstronomyDynamical mass generationGauge-invarianceSchwinger–Dyson equationsRenormalizationTheoretical physicsQuantization (physics)symbols.namesakeHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Non-Abelian gauge theoriesFeynman diagramGauge theoryGauge bosonsQuantum chromodynamicsPhysicsBackground field methodGreens functionsElectroweak interactionHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbols
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Small and hollow magnetic monopoles

2018

We deal with the presence of magnetic monopoles in a non Abelian model that generalizes the standard 't~Hooft-Polyakov model in three spatial dimensions. We investigate the energy density of the static and spherically symmetric solutions to find first order differential equations that solve the equations of motion. The system is further studied and two distinct classes of solutions are obtained, one that can also be described by analytical solutions which is called small monopole, since it is significantly smaller than the standard 't~Hooft-Polyakov monopole. The other type of structure is the hollow monopole, since the energy density is endowed with a hole at its core. The hollow monopole …

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsDifferential equationHigh Energy Physics::LatticeMathematical analysisMagnetic monopoleStructure (category theory)FOS: Physical sciencesEquations of motionPattern Formation and Solitons (nlin.PS)Type (model theory)Nonlinear Sciences - Pattern Formation and Solitons01 natural sciencesCondensed Matter - Other Condensed MatterCore (optical fiber)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Ordinary differential equation0103 physical sciencesEnergy density010306 general physicsOther Condensed Matter (cond-mat.other)Physical Review D
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Supersymmetry from boundary conditions

2004

We study breaking and restoration of supersymmetry in five-dimensional theories by determining the mass spectrum of fermions from their equations of motion. Boundary conditions can be obtained from either the action principle by extremizing an appropriate boundary action (interval approach) or by assigning parities to the fields (orbifold approach). In the former, fields extend continuously from the bulk to the boundaries, while in the latter the presence of brane mass-terms cause fields to jump when one moves across the branes. We compare the two approaches and in particular we carefully compute the non-trivial jump profiles of the wavefunctions in the orbifold picture for very general bra…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesEquations of motionFermionSupersymmetryHigh Energy Physics::TheoryTheoretical physicsHigh Energy Physics - Theory (hep-th)Differential geometryQuantum mechanicsBrane cosmologyBoundary value problemBraneOrbifoldNuclear Physics B
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Aspects of D-brane Dynamics in Supergravity Backgrounds with Fluxes, Kappa-symmetry and Equations of Motion. Part IIB

2006

We derive and carry out a detailed analysis of the equations of motion of the type IIB D branes in generic supergravity backgrounds with fluxes making account of the worldvolume Born-Infeld gauge field and putting a special emphasis on the structure of the Dirac equation for Dp brane fermionic modes. We present an explicit form of the worldvolume field equations for each of the Dp branes (p=1,3,5,7,9) in the cases in which the Neveu-Schwarz flux and the Ramond-Ramond p-form flux along the Dp-brane worldvolume are zero and the supergravity backgrounds do not necessarily induce the worldvolume Born-Infeld flux. We then give several examples of D3, D5 and D7 brane configurations in which the w…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsInstantonCompactification (physics)SupergravityEquations of motionFOS: Physical sciencessymbols.namesakeHigh Energy Physics::TheoryClassical mechanicsHigh Energy Physics - Theory (hep-th)Mathematics::K-Theory and HomologyDirac equationsymbolsBrane cosmologyGauge theoryD-braneMathematical physics
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