Search results for "ExAC"

showing 10 items of 1440 documents

The Complete Solution of the Classical SL(2,ℝ/U(1) Gauged WZNW Field Theory

1998

We prove that any gauged WZNW model has a Lax pair representation, and give explicitly the general solution of the classical equations of motion of the SL(2,R)/U(1) theory. We calculate the symplectic structure of this solution by solving a differential equation of the Gelfand-Dikii type with initial state conditions at infinity, and transform the canonical physical fields non-locally onto canonical free fields. The results will, finally, be collected in a local B\"acklund transformation. These calculations prepare the theory for an exact canonical quantization.

High Energy Physics - TheoryDifferential equationCanonical quantizationFOS: Physical sciencesEquations of motionStatistical and Nonlinear PhysicsState (functional analysis)Type (model theory)Nonlinear Sciences::Exactly Solvable and Integrable SystemsHigh Energy Physics - Theory (hep-th)Lax pairField theory (psychology)Mathematical PhysicsSymplectic geometryMathematical physicsMathematicsCommunications in Mathematical Physics
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Space-like (vs. time-like) collinear limits in QCD: Is factorization violated?

2012

We consider the singular behaviour of QCD scattering amplitudes in kinematical configurations where two or more momenta of the external partons become collinear. At the tree level, this behaviour is known to be controlled by factorization formulae in which the singular collinear factor is universal (process independent). We show that this strict (process-independent) factorization is not valid at one-loop and higher-loop orders in the case of the collinear limit in space-like regions (e.g., collinear radiation from initial-state partons). We introduce a generalized version of all-order collinear factorization, in which the space-like singular factors retain some dependence on the momentum a…

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesPartonSpace (mathematics)01 natural sciences//purl.org/becyt/ford/1 [https]MomentumHigh Energy Physics - Phenomenology (hep-ph)Factorization0103 physical sciences010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsFísicaCharge (physics)//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Gravitational singularityCIENCIAS NATURALES Y EXACTAS
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Double collinear splitting amplitudes at next-to-leading order

2013

We compute the next-to-leading order (NLO) QCD corrections to the $1 \to 2$ splitting amplitudes in different dimensional regularization (DREG) schemes. Besides recovering previously known results, we explore new DREG schemes and analyze their consistency by comparing the divergent structure with the expected behavior predicted by Catani's formula. Through the introduction of scalar-gluons, we show the relation among splittings matrices computed using different schemes. Also, we extended this analysis to cover the double collinear limit of scattering amplitudes in the context of QCD+QED.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]Dimensional regularizationHigh Energy Physics - Phenomenology (hep-ph)Consistency (statistics)0103 physical sciencesLimit (mathematics)010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Cover (topology)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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Triple collinear splitting functions at NLO for scattering processes with photons

2014

We present splitting functions in the triple collinear limit at next-to-leading order. The computation was performed in the context of massless QCD+QED, considering only processes which include at least one photon. Through the comparison of the IR divergent structure of splitting amplitudes with the expected known behavior, we were able to check our results. Besides that we implemented some consistency checks based on symmetry arguments and cross-checked the results among them. Studying photon-started processes, we obtained very compact results.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsPhotonCiencias FísicasComputationFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsScatteringFísica//purl.org/becyt/ford/1.3 [https]Symmetry (physics)AstronomíaMassless particleHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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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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Exact spherically-symmetric inhomogeneous model withnperfect fluids

2011

We present the exact equations governing the dynamics of a spherically-symmetric inhomogeneous model with n decoupled and non-comoving perfect fluids. Thanks to the use of physically meaningful quantities we write the set of 3+2n equations in a concise and transparent way. The n perfect fluids can have general equations of state, thus making the model extremely flexible to study a large variety of cosmological and astrophysical problems. As applications we consider a model sourced by two non-comoving dust components and a cosmological constant, and a model featuring dust and a dark energy component with negligible speed of sound.

High Energy Physics - TheoryPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterFOS: Physical sciencesExact differential equationAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsCosmological constant01 natural sciencesGeneral Relativity and Quantum CosmologySymmetry (physics)CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Speed of sound0103 physical sciencesDark energyCosmological perturbation theory010303 astronomy & astrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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What is a singular black hole beyond general relativity?

2017

Exploring the characterization of singular black hole spacetimes, we study the relation between energy density, curvature invariants, and geodesic completeness using a quadratic $f(R)$ gravity theory coupled to an anisotropic fluid. Working in a metric-affine approach, our models and solutions represent minimal extensions of General Relativity (GR) in the sense that they rapidly recover the usual Reissner-Nordstr\"{o}m solution from near the inner horizon outwards. The anisotropic fluid helps modify only the innermost geometry. Depending on the values and signs of two parameters on the gravitational and matter sectors, a breakdown of the correlations between the finiteness/divergence of the…

High Energy Physics - TheoryPhysicsMODIFIED THEORIES OF GRAVITY010308 nuclear & particles physicsGeneral relativityCiencias FísicasFOS: Physical sciences//purl.org/becyt/ford/1.3 [https]General Relativity and Quantum Cosmology (gr-qc)COSMIC CENSORSHIPOtras Ciencias Físicas01 natural sciencesCLASSICAL BLACK HOLESGeneral Relativity and Quantum Cosmology//purl.org/becyt/ford/1 [https]General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)EINSTEIN-MAXWELL SPACETIMEQuantum mechanics0103 physical sciences010306 general physicsHumanitiesCIENCIAS NATURALES Y EXACTASPhysical Review D
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Abelian current algebra and the Virasoro algebra on the lattice

1993

We describe how a natural lattice analogue of the abelian current algebra combined with free discrete time dynamics gives rise to the lattice Virasoro algebra and corresponding hierarchy of conservation laws.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsConservation lawPure mathematicsHigh Energy Physics::Lattice010102 general mathematicsCurrent algebraFOS: Physical sciences01 natural sciencesNonlinear Sciences::Exactly Solvable and Integrable SystemsHigh Energy Physics - Theory (hep-th)Discrete time and continuous timeLattice (order)0103 physical sciencesVirasoro algebra0101 mathematicsAbelian group010306 general physicsPhysics Letters B
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Supersymmetry in non commutative superspaces

2003

Non commutative superspaces can be introduced as the Moyal-Weyl quantization of a Poisson bracket for classical superfields. Different deformations are studied corresponding to constant background fields in string theory. Supersymmetric and non supersymmetric deformations can be defined, depending on the differential operators used to define the Poisson bracket. Some examples of deformed, 4 dimensional lagrangians are given. For extended superspace (N>1), some new deformations can be defined, with no analogue in the N=1 case.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesFísicaSupersymmetrySuperspaceString theoryDifferential operatorNoncommutative geometryPoisson bracketQuantization (physics)High Energy Physics::TheoryNonlinear Sciences::Exactly Solvable and Integrable SystemsHigh Energy Physics - Theory (hep-th)Commutative propertyComputer Science::DatabasesParticle Physics - TheoryMathematical 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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