Search results for "PERTURBATION"

showing 10 items of 811 documents

Direct perturbation theory in terms of energy derivatives: Fourth-order relativistic corrections at the Hartree–Fock level

2011

In this work, the quantum-chemical treatment of relativistic effects by means of direct perturbation theory is extended from its lowest order, DPT2, to the next higher order, DPT4. The required theory is given in terms of energy derivatives with the DPT4 energy correction defined as the corresponding second derivative with respect to the relativistic perturbation parameter λ(rel) = c(2) and c as the speed of light. To facilitate the implementation in standard quantum-chemical program packages, a general formulation of DPT starting from a nonrelativistic Lagrangian is developed, thereby expanding both wave function and operators in terms of λ(rel). The corresponding expressions, which incorp…

PhysicsHartree–Fock methodGeneral Physics and AstronomyPerturbation (astronomy)symbols.namesakeFourth orderModels ChemicalQuantum electrodynamicssymbolsQuantum TheoryPhysical and Theoretical ChemistryRelativistic quantum chemistryWave functionHyperfine structureSoftwareLagrangianSecond derivativeThe Journal of Chemical Physics
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Analytic form of the full two-loop five-gluon all-plus helicity amplitude

2019

We compute the full-color two-loop five-gluon amplitude for the all-plus helicity configuration. In order to achieve this, we calculate the required master integrals for all permutations of the external legs, in the physical scattering region. We verify the expected divergence structure of the amplitude, and extract the finite hard function. We further validate our result by checking the factorization properties in the collinear limit. Our result is fully analytic and valid in the physical scattering region. We express it in a compact form containing logarithms, dilogarithms and rational functions.

PhysicsHigh Energy Physics - Theory530 PhysicsMathematical analysisGeneral Physics and AstronomyFOS: Physical sciences10192 Physics InstituteRational functionFunction (mathematics)01 natural sciencesHelicity3100 General Physics and AstronomyHigh Energy Physics - Phenomenology; High Energy Physics - Phenomenology; High Energy Physics - TheoryScattering amplitudeHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Phenomenology (hep-ph)FactorizationHigh Energy Physics - Theory (hep-th)0103 physical sciencesGauge theories Perturbation theory Perturbative QCD Scattering amplitudes GluonsPerturbation theory (quantum mechanics)Limit (mathematics)010306 general physics
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Cosmological Perturbations in Renormalization Group Derived Cosmologies

2002

A linear cosmological perturbation theory of an almost homogeneous and isotropic perfect fluid Universe with dynamically evolving Newton constant $G$ and cosmological constant $\Lambda$ is presented. A gauge-invariant formalism is developed by means of the covariant approach, and the acoustic propagation equations governing the evolution of the comoving fractional spatial gradients of the matter density, $G$, and $\Lambda$ are thus obtained. Explicit solutions are discussed in cosmologies where both $G$ and $\Lambda$ vary according to renormalization group equations in the vicinity of a fixed point.

PhysicsHigh Energy Physics - TheoryIsotropyAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsPerfect fluidCosmological constantAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsFixed pointRenormalization groupAstrophysicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceHomogeneousCosmological perturbation theoryCovariant transformationMathematical PhysicsMathematical physics
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Hamiltonian lattice QCD at finite density: equation of state in the strong coupling limit

2001

The equation of state of Hamiltonian lattice QCD at finite density is examined in the strong coupling limit by constructing a solution to the equation of motion corresponding to an effective Hamiltonian describing the ground state of the many body system. This solution exactly diagonalizes the Hamiltonian to second order in field operators for all densities and is used to evaluate the vacuum energy density from which we obtain the equation of state. We find that up to and beyond the chiral symmetry restoration density the pressure of the quark Fermi sea can be negative indicating its mechanical instability. Our result is in qualitative agreement with continuum models and should be verifiabl…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsChiral perturbation theoryNuclear TheoryHigh Energy Physics::LatticeLattice field theoryQCD vacuumAstrophysics (astro-ph)High Energy Physics - Lattice (hep-lat)FOS: Physical sciencesLattice QCDAstrophysicsNuclear Theory (nucl-th)symbols.namesakeHigh Energy Physics - PhenomenologyHamiltonian lattice gauge theoryHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeHigh Energy Physics - Theory (hep-th)Quantum electrodynamicssymbolsHamiltonian (quantum mechanics)Ground stateLattice model (physics)
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Resizing the Conformal Window: A beta function Ansatz

2009

We propose an ansatz for the nonperturbative beta function of a generic non-supersymmetric Yang-Mills theory with or without fermions in an arbitrary representation of the gauge group. While our construction is similar to the recently proposed Ryttov-Sannino all order beta function, the essential difference is that it allows for the existence of an unstable ultraviolet fixed point in addition to the predicted Bank-Zaks -like infrared stable fixed point. Our beta function preserves all of the tested features with respect to the non-supersymmetric Yang-Mills theories. We predict the conformal window identifying the lower end of it as a merger of the infrared and ultraviolet fixed points.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesConformal mapSupersymmetryFunction (mathematics)Astrophysics::Cosmology and Extragalactic AstrophysicsFixed pointTheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryClassical mechanicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Gauge groupGauge theoryPerturbation theory (quantum mechanics)Ansatz
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The H-graph with equal masses in terms of multiple polylogarithms

2021

The initial phase of the inspiral process of a binary system producing gravitational waves can be described by perturbation theory. At the third post-Minkowskian order a two-loop double box graph, known as H-graph contributes. We consider the case where the two objects making up the binary system have equal masses. We express all master integrals related to the equal-mass H-graph up to weight four in terms of multiple polylogarithms. We provide a numerical program which evaluates all master integrals up to weight four in the physical regions with arbitrary precision.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsPure mathematics010308 nuclear & particles physicsGravitational wavePhysicsQC1-999Process (computing)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Initial phase0103 physical sciencesArbitrary-precision arithmeticGraph (abstract data type)Order (group theory)Binary systemPerturbation theory (quantum mechanics)010306 general physics
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Metric-Palatini gravity unifying local constraints and late-time cosmic acceleration

2011

We present a novel approach to modified theories of gravity that consists of adding to the Einstein-Hilbert Lagrangian an f(R) term constructed a la Palatini. Using the respective dynamically equivalent scalar-tensor representation, we show that the theory can pass the Solar System observational constraints even if the scalar field is very light. This implies the existence of a long-range scalar field, which is able to modify the cosmological and galactic dynamics, but leaves the Solar System unaffected. We also verify the absence of instabilities in perturbations and provide explicit models which are consistent with local tests and lead to the late-time cosmic acceleration.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsSolar SystemCosmology and Nongalactic Astrophysics (astro-ph.CO)COSMIC cancer database010308 nuclear & particles physicsFOS: Physical sciencesPerturbation (astronomy)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesCosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencessymbolsf(R) gravity010306 general physicsScalar fieldLagrangianAstrophysics - Cosmology and Nongalactic Astrophysics
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Quasidisks and string theory

1990

Abstract A heuristic model of non-perturbative bosonic string theory on the Bers universal Teichmuller space of normalized quasidisks is discussed. It is suggested that the infinite-dimensional analogue of the Polyakov energy might be the quasidisk area.

PhysicsHigh Energy Physics::TheoryNuclear and High Energy PhysicsNon-critical string theoryMathematics::Complex VariablesHeuristicBosonic string theoryStability (learning theory)Universal Teichmüller spaceVirasoro algebraPerturbation theory (quantum mechanics)String theoryMathematical physicsPhysics Letters B
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Baryon chiral perturbation theory

2009

We provide a short introduction to the one-nucleon sector of chiral perturbation theory and address the issue of power counting and renormalization. We discuss the infrared regularization and the extended on-mass-shell scheme. Both allow for the inclusion of further degrees of freedom beyond pions and nucleons and the application to higher-loop calculations. As applications we consider the chiral expansion of the nucleon mass to order ${\cal O}(q^6)$ and the inclusion of vector and axial-vector mesons in the calculation of nucleon form factors. Finally, we address the complex-mass scheme for describing unstable particles in effective field theory.

PhysicsHistoryChiral perturbation theoryNuclear TheoryMesonHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyHigh Energy Physics - Lattice (hep-lat)Nuclear TheoryDegrees of freedom (statistics)FOS: Physical sciencesComputer Science ApplicationsEducationNuclear Theory (nucl-th)BaryonRenormalizationHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)PionRegularization (physics)Effective field theoryNuclear ExperimentNucleonJournal of Physics: Conference Series
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Ionization of atomic hydrogen with up to four excess photons by circularly and linearly polarized light

2012

The above threshold ionization (ATI) is investigated for H in ns states. The total generalized cross sections are calculated for up to 4 excess photons using perturbation theory and modified Coulomb Green's function Sturmian expansion.

PhysicsHistoryPhotonHydrogenLinearly polarized lightAbove threshold ionizationchemistry.chemical_elementFunction (mathematics)Computer Science ApplicationsEducationchemistryIonizationCoulombPhysics::Atomic PhysicsAtomic physicsPerturbation theoryJournal of Physics: Conference Series
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