Search results for "Nuclear and high energy physics"

showing 10 items of 8241 documents

Hairy black-holes in shift-symmetric theories

2020

Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem of Hui and Nicolis, assuming spherical symmetry, time-independence of the scalar field and asymptotic flatness. The most studied counterexample is a linear coupling of the scalar with the Gauss-Bonnet invariant. However, in this case the norm of the shift-symmetry current $J^2$ diverges at the horizon casting doubts on whether the solution is physically sound. We show that this is not an issue since $J^2$ is not a scalar quantity, since $J^\mu$ is not a diff-invariant current in the presence of Gauss-Bonnet. The same theory can be written in Horndeski form with a non-analytic function $G_5 \s…

High Energy Physics - TheoryNuclear and High Energy PhysicsBlack HolesCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysical quantityMathematical physicsPhysics010308 nuclear & particles physicsScalar (physics)Black HoleInvariant (physics)Linear couplingSettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciHigh Energy Physics - Theory (hep-th)astro-ph.COlcsh:QC770-798Circular symmetryScalar fieldClassical Theories of GravityAstrophysics - Cosmology and Nongalactic AstrophysicsCounterexample
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Matter dependence of the four-loop QCD cusp anomalous dimension: from small angles to all angles

2019

We compute the fermionic contributions to the cusp anomalous dimension in QCD at four loops as an expansion for small cusp angle. As a byproduct we also obtain the respective terms of the four-loop HQET wave function anomalous dimension. Our new results at small angles provide stringent tests of a recent conjecture for the exact angle dependence of the matter terms in the four-loop cusp anomalous dimension. We find that the conjecture does not hold for two of the seven fermionic color structures, but passes all tests for the remaining terms. This provides strong support for the validity of the corresponding conjectured expressions with full angle dependence. Taking the limit of large Minkow…

High Energy Physics - TheoryNuclear and High Energy PhysicsConformal anomalyFOS: Physical sciencesConformal map01 natural sciencesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Dimension (vector space)Perturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityScattering Amplitudes010306 general physicsWave functionQuantum chromodynamicsCusp (singularity)Physics010308 nuclear & particles physicsPerturbative QCDEffective Field TheoriesWilson ’t Hooft and Polyakov loopsScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Journal of High Energy Physics
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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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Chirality transfer and chiral turbulence in gauge theories

2020

Chirality transfer between fermions and gauge fields plays a crucial role for understanding the dynamics of anomalous transport phenomena such as the Chiral Magnetic Effect. In this proceeding we present a first principles study of these processes based on classical-statistical real-time lattice simulations of strongly coupled QED $(e^2N_f=64)$. Our simulations demonstrate that a chirality imbalance in the fermion sector triggers chiral plasma instabilities in the gauge field sector, which ultimately lead to the generation of long range helical magnetic fields via a self-similar turbulent cascade of the magnetic helicity.

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)High Energy Physics::Latticechiral plasma instabilitiesFOS: Physical sciences01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Magnetic helicity0103 physical sciencesGauge theory010306 general physicsPhysicsChirality transferchiral turbulence010308 nuclear & particles physicsmagnetogensisHigh Energy Physics::PhenomenologyFermionPlasmaMagnetic fieldHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)CascadeQuantum electrodynamicsChirality (chemistry)Transport phenomenaAstrophysics - Cosmology and Nongalactic Astrophysics
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Tensor bounds on the hidden universe

2018

During single clock inflation, hidden fields (i.e. fields coupled to the inflaton only gravitationally) in their adiabatic vacua can ordinarily only affect observables through virtual effects. After renormalizing background quantities (fixed by observations at some pivot scale), all that remains are logarithmic runnings in correlation functions that are both Planck and slow roll suppressed. In this paper we show how a large number of hidden fields can partially compensate this suppression and generate a potentially observable running in the tensor two point function, consistently inferable courtesy of a large $N$ resummation. We detour to address certain subtleties regarding loop correction…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)ddc:500.201 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityTensorPlanck010306 general physicsmedia_commonPhysicsInflation (cosmology)Slow roll010308 nuclear & particles physicsScalar (physics)InflatonCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Renormalization Regularization and RenormalonsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Non-equilibrium dynamics of a scalar field with quantum backreaction

2021

We study the dynamical evolution of coupled one- and two-point functions of a scalar field in the 2PI framework at the Hartree approximation, including backreaction from out-of-equilibrium modes. We renormalize the 2PI equations of motion in an on-shell scheme in terms of physical parameters. We present the Hartree-resummed renormalized effective potential at finite temperature and critically discuss the role of the effective potential in a non-equilibrium system. We follow the decay and thermalization of a scalar field from an initial cold state with all energy stored in the potential, into a fully thermalized system with a finite temperature. We identify the non-perturbative processes of …

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)quantum dissipative systemsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)QC770-798hiukkasfysiikkakosmologia114 Physical sciences01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesThermal Field Theory010306 general physics010308 nuclear & particles physicsthermal field theoryHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Nonperturbative Effectsnonperturbative effectskvanttikenttäteoriaQuantum Dissipative SystemsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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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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BASIC TWIST QUANTIZATION OF osp(1|2) AND κ-DEFORMATION OF D = 1 SUPERCONFORMAL MECHANICS

2003

The twisting function describing a nonstandard (super-Jordanian) quantum deformation of $osp(1|2)$ is given in explicite closed form. The quantum coproducts and universal R-matrix are presented. The non-uniqueness of the twisting function as well as two real forms of the deformed $osp(1|2)$ superalgebras are considered. One real quantum $osp(1|2)$ superalgebra is interpreted as describing the $\kappa$-deformation of D=1, N=1 superconformal algebra, which can be applied as a symmetry algebra of N=1 superconformal mechanics.

High Energy Physics - TheoryNuclear and High Energy PhysicsFOS: Physical sciencesGeneral Physics and AstronomyHigh Energy Physics::TheoryQuantization (physics)Mathematics::Quantum AlgebraMathematics - Quantum AlgebraFOS: MathematicsQuantum Algebra (math.QA)Representation Theory (math.RT)TwistMathematics::Representation TheoryQuantumMathematical PhysicsPhysicsAstronomy and AstrophysicsMathematical Physics (math-ph)SupersymmetryFunction (mathematics)MechanicsSuperalgebraSymmetry (physics)High Energy Physics - Theory (hep-th)Superconformal algebraMathematics - Representation TheoryModern Physics Letters A
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Complete integration-by-parts reductions of the non-planar hexagon-box via module intersections

2018

We present the powerful module-intersection integration-by-parts (IBP) method, suitable for multi-loop and multi-scale Feynman integral reduction. Utilizing modern computational algebraic geometry techniques, this new method successfully trims traditional IBP systems dramatically to much simpler integral-relation systems on unitarity cuts. We demonstrate the power of this method by explicitly carrying out the complete analytic reduction of two-loop five-point non-planar hexagon-box integrals, with degree-four numerators, to a basis of 73 master integrals.

High Energy Physics - TheoryNuclear and High Energy PhysicsFeynman integralFOS: Physical sciencesAlgebraic geometryTopologyDifferential and Algebraic Geometry; Scattering Amplitudes; Perturbative QCD01 natural sciencesSubatomär fysikReduction (complexity)Mathematics - Algebraic GeometryPlanarHigh Energy Physics - Phenomenology (hep-ph)Subatomic Physics0103 physical sciencesPerturbative QCDFOS: MathematicsIntegration by partsDifferential and Algebraic Geometrylcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsScattering AmplitudesAlgebraic Geometry (math.AG)PhysicsBasis (linear algebra)Unitarity010308 nuclear & particles physicsPower (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Journal of High Energy Physics
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Implications of nonplanar dual conformal symmetry

2018

Recently, Bern et al observed that a certain class of next-to-planar Feynman integrals possess a bonus symmetry that is closely related to dual conformal symmetry. It corresponds to a projection of the latter along a certain lightlike direction. Previous studies were performed at the level of the loop integrand, and a Ward identity for the integral was formulated. We investigate the implications of the symmetry at the level of the integrated quantities. In particular, we focus on the phenomenologically important case of five-particle scattering. The symmetry simplifies the four-variable problem to a three-variable one. In the context of the recently proposed space of pentagon functions, the…

High Energy Physics - TheoryNuclear and High Energy PhysicsFunction spaceFeynman graphFOS: Physical sciencesanomalyContext (language use)Ward identitySpace (mathematics)Conformal and W Symmetry01 natural sciencesProjection (linear algebra)Identity (mathematics)High Energy Physics - Phenomenology (hep-ph)Conformal symmetry0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityAnomalies in Field and String Theories010306 general physicsScattering AmplitudesParticle Physics - PhenomenologyMathematical physicsPhysicsloop integral010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thscattering amplitudehep-phSymmetry (physics)Loop (topology)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symmetry: conformalsupersymmetry: 4[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798dualityParticle Physics - Theoryinfrared problem
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