Search results for "Riemann hypothesis"

showing 10 items of 31 documents

Degenerate Riemann theta functions, Fredholm and wronskian representations of the solutions to the KdV equation and the degenerate rational case

2021

International audience; We degenerate the finite gap solutions of the KdV equation from the general formulation given in terms of abelian functions when the gaps tend to points, to get solutions to the KdV equation given in terms of Fredholm determinants and wronskians. For this we establish a link between Riemann theta functions, Fredholm determinants and wronskians. This gives the bridge between the algebro-geometric approach and the Darboux dressing method.We construct also multi-parametric degenerate rational solutions of this equation.

KdV equationPure mathematicsGeneral Physics and AstronomyFredholm determinantTheta function01 natural sciencessymbols.namesakeWronskians[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]Fredholm determinant0103 physical sciencesRiemann theta functions0101 mathematicsAbelian group010306 general physicsKorteweg–de Vries equationMathematical PhysicsMathematicsWronskianRiemann surface010102 general mathematicsDegenerate energy levelsRiemann hypothesisNonlinear Sciences::Exactly Solvable and Integrable SystemsRiemann surfacesymbolsGeometry and Topology
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Historischer Überblick zur mathematischen Theorie von Unstetigkeitswellen seit Riemann und Christoffel

1981

We give a brief historical account of the development of the mathematical theory of propagation of discontinuities in gases, fluids or elastic materials. The theory was initiated by Riemann who investigated the propagation of shocks in one-dimensional isentropic gas flow. Riemann’s results were used by Christoffel to treat, more generally, the propagation of (first order) discontinuity surfaces in three-dimensional flows of perfect fluids. Subsequently Christoffel applied his general theory to first order waves in certain elastic materials. Independently of Riemann and Christoffel significant contributions were made by Hugoniot. The theory was completed in Hadamard’s celebrated monograph [3…

Mathematical theoryConservation lawRiemann hypothesissymbols.namesakeDiscontinuity (linguistics)Christoffel symbolsFlow (mathematics)Hyperelastic materialMathematical analysissymbolsInitial value problemMathematics
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Algebraic Curves and Riemann Surfaces in Matlab

2010

In the previous chapter, a detailed description of the algorithms for the ‘algcurves’ package in Maple was presented. As discussed there, the package is able to handle general algebraic curves with coefficients given as exact arithmetic expressions, a restriction due to the use of exact integer arithmetic. Coefficients in terms of floating point numbers, i.e., the representation of decimal numbers of finite length on a computer, can in principle be handled, but the floating point numbers have to be converted to rational numbers. This can lead to technical difficulties in practice. One also faces limitations if one wants to study families of Riemann surfaces, where the coefficients in the al…

Moduli of algebraic curvesAlgebraRiemann–Hurwitz formulaRiemann hypothesissymbols.namesakeGeometric function theoryRiemann surfaceComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATIONAlgebraic surfacesymbolsRiemann's differential equationBranch pointMathematics
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Meson-Baryon Interactions in Unitarized Chiral Perturbation Theory

2002

Meson-Baryon Interactions can be successfully described using both Chiral Symmetry and Unitarity. The $s-$wave meson-baryon scattering amplitude is analyzed in a Bethe-Salpeter coupled channel formalism incorporating Chiral Symmetry in the potential. Two body coupled channel unitarity is exactly preserved. The needed two particle irreducible matrix amplitude is taken from lowest order Chiral Perturbation Theory in a relativistic formalism. Off-shell behavior is parameterized in terms of low energy constants. The relation to the heavy baryon limit is discussed. The position of the complex poles in the second Riemann sheet of the scattering amplitude determine masses and widths baryonic reson…

PhysicsChiral perturbation theoryNuclear TheoryMesonUnitarityNuclear TheoryHigh Energy Physics::PhenomenologyFOS: Physical sciencesLambdaBaryonScattering amplitudeNuclear Theory (nucl-th)Riemann hypothesissymbols.namesakeAmplitudesymbolsNuclear ExperimentMathematical physics
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On Riemann’s Ideas on Space and Schwinger’s Treatment of Low-Energy Pion-Nucleon Physics

2020

We begin with a demonstration of how great an influence Riemann’s habilitation essay had on the development of field theory. His ideas about the origin of physical space and the importance of a metric field were clearly outlined as early as 1854, and praised highly by the old C.F. Gauss, who died 1 year later. There is but one formula in Riemann’s article. This formula and its relevance will be explained at the beginning of the present chapter. The basic principle which is omnipresent in Riemann’s entire work is to understand the physical behavior of nature from its smallness. Hence partial differential equations stand at the beginning of any field theory. In our case, it is not the metric …

PhysicsField (physics)InfinitesimalGausseducation.educational_degreeSpace (mathematics)Action (physics)HabilitationRiemann hypothesissymbols.namesakeTheoretical physicssymbolsField theory (psychology)education
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Numerical 3+1 general relativistic magnetohydrodynamics: a local characteristic approach

2005

We present a general procedure to solve numerically the general relativistic magnetohydrodynamics (GRMHD) equations within the framework of the 3+1 formalism. The work reported here extends our previous investigation in general relativistic hydrodynamics (Banyuls et al. 1997) where magnetic fields were not considered. The GRMHD equations are written in conservative form to exploit their hyperbolic character in the solution procedure. All theoretical ingredients necessary to build up high-resolution shock-capturing schemes based on the solution of local Riemann problems (i.e. Godunov-type schemes) are described. In particular, we use a renormalized set of regular eigenvectors of the flux Jac…

PhysicsGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyMagnetic fieldRiemann hypothesissymbols.namesakeClassical mechanicsRotating black holeSpace and Planetary ScienceMagnetorotational instabilitysymbolsSchwarzschild metricMagnetohydrodynamicsEigenvalues and eigenvectors
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An introduction to relativistic hydrodynamics

2007

We review formulations of the equations of (inviscid) general relativistic hydrodynamics and (ideal) magnetohydrodynamics, along with methods for their numerical solution. Both systems can be cast as first-order, hyperbolic systems of conservation laws, following the explicit choice of an Eulerian observer and suitable fluid and magnetic field variables. During the last fifteen years, the so-called (upwind) high-resolution shock-capturing schemes based on Riemann solvers have been successfully extended from classical to relativistic fluid dynamics, both special and general. Nowadays, general relativistic hydrodynamical simulations in relativistic astrophysics are routinely performed, partic…

PhysicsHistoryConservation lawGeneral relativitySpace timeEulerian pathComputer Science ApplicationsEducationMagnetic fieldsymbols.namesakeRiemann hypothesisClassical mechanicsInviscid flowsymbolsMagnetohydrodynamicsJournal of Physics: Conference Series
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Precise determination of resonance pole parameters through Pad\'e approximants

2014

In this work, we present a precise and model--independent method to extract resonance pole parameters from phase-shift scattering data. These parameters are defined from the associated poles in the second Riemann sheet, unfolded by the analytic continuation to the complex pole using Pad\'e approximants. Precise theoretical parameterizations of pion-pion scattering phase shifts based on once-- and twice-- subtracted dispersion relations are used as input, whose functional form allows us to show the benefit and accuracy of the method. In particular, we extract from these parametrization the pole positions of the $f_0(500)$ at $\sqrt{s}=(453\pm 15) - i(297 \pm 15)$ MeV, the $\rho(770)$ at $\sq…

PhysicsNuclear and High Energy PhysicsParticle physicsMesonNuclear TheoryScatteringAnalytic continuationResonanceRiemann hypothesissymbols.namesakeHigh Energy Physics - PhenomenologyPionHigh Energy Physics - LatticeQuantum electrodynamicsDispersion relationsymbolsPadé approximantNuclear Experiment
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Numerical Hydrodynamics in General Relativity

2003

The current status of numerical solutions for the equations of ideal general relativistic hydrodynamics is reviewed. With respect to an earlier version of the article the present update provides additional information on numerical schemes and extends the discussion of astrophysical simulations in general relativistic hydrodynamics. Different formulations of the equations are presented, with special mention of conservative and hyperbolic formulations well-adapted to advanced numerical methods. A large sample of available numerical schemes is discussed, paying particular attention to solution procedures based on schemes exploiting the characteristic structure of the equations through lineariz…

PhysicsNumerical RelativityField (physics)Physics and Astronomy (miscellaneous)General relativityNumerical analysisAstrophysics (astro-ph)Structure (category theory)FOS: Physical sciencesReview ArticleGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysicslcsh:Atomic physics. Constitution and properties of matterGeneral Relativity and Quantum Cosmologylcsh:QC170-197Neutron starRiemann hypothesissymbols.namesakeClassical mechanicsGravitational fieldGravitational collapsesymbolsLiving Reviews in Relativity
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Type D vacuum solutions: a new intrinsic approach

2013

We present a new approach to the intrinsic properties of the type D vacuum solutions based on the invariant symmetries that these spacetimes admit. By using tensorial formalism and without explicitly integrating the field equations, we offer a new proof that the upper bound of covariant derivatives of the Riemann tensor required for a Cartan-Karlhede classification is two. Moreover we show that, except for the Ehlers-Kundt's C-metrics, the Riemann derivatives depend on the first order ones, and for the C-metrics they depend on the first order derivatives and on a second order constant invariant. In our analysis the existence of an invariant complex Killing vector plays a central role. It al…

PhysicsRiemann curvature tensorPure mathematicsPhysics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)Upper and lower boundsGeneral Relativity and Quantum Cosmologysymbols.namesakeRiemann hypothesisKilling vector fieldGeneral Relativity and Quantum CosmologyHomogeneous spacesymbolsCovariant transformationField equation
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