Search results for "RIEMANN"

showing 10 items of 254 documents

Birkhoff theorem and conformal Killing-Yano tensors

2015

We analyze the main geometric conditions imposed by the hypothesis of the Jebsen-Birkhoff theorem. We show that the result (existence of an additional Killing vector) does not necessarily require a three-dimensional isometry group on two-dimensional orbits but only the existence of a conformal Killing-Yano tensor. In this approach the (additional) isometry appears as the known invariant Killing vector that the ${\cal D}$-metrics admit.

PhysicsKilling vector fieldPure mathematicsGeneral Relativity and Quantum CosmologyPhysics and Astronomy (miscellaneous)FOS: Physical sciencesConformal mapTensorGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (mathematics)Isometry groupIsometry (Riemannian geometry)General Relativity and Quantum Cosmology
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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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Anomalous chiral perturbation theory meson Lagrangian to orderp6reexamined

2002

We present a revised and extended construction of the mesonic Lagrangian density in chiral perturbation theory (ChPT) at order ${p}^{6}$ in the anomalous (or epsilon) sector, ${\mathcal{L}}_{6,\ensuremath{\epsilon}}.$ After improving several aspects of the strategy we used originally, i.e., a more efficient application of partial integration, the implementation of so-called Bianchi identities, and additional trace relations, we find the new monomial sets to include 24 ${SU(N}_{f}),$ 23 $\mathrm{SU}(3),$ and 5 $\mathrm{SU}(2)$ elements. Furthermore, we introduce 8 supplementary terms due to the extension of the chiral group to ${SU(N}_{f}{)}_{L}\ifmmode\times\else\texttimes\fi{}{SU(N}_{f}{)}…

PhysicsNuclear and High Energy PhysicsRiemann curvature tensorParticle physicsMonomialChiral perturbation theoryTrace (linear algebra)Meson010308 nuclear & particles physicsGroup (mathematics)Order (ring theory)01 natural sciencessymbols.namesake0103 physical sciencessymbols010306 general physicsLagrangianMathematical physicsPhysical Review D
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The unequal mass sunrise integral expressed through iterated integrals on M‾1,3

2020

Abstract We solve the two-loop sunrise integral with unequal masses systematically to all orders in the dimensional regularisation parameter e. In order to do so, we transform the system of differential equations for the master integrals to an e-form. The sunrise integral with unequal masses depends on three kinematical variables. We perform a change of variables to standard coordinates on the moduli space M 1 , 3 of a genus one Riemann surface with three marked points. This gives us the solution as iterated integrals on M ‾ 1 , 3 . On the hypersurface τ = const our result reduces to elliptic polylogarithms. In the equal mass case our result reduces to iterated integrals of modular forms.

PhysicsNuclear and High Energy Physicssymbols.namesakeChange of variablesHypersurfaceDifferential equationRiemann surfaceGenus (mathematics)Mathematical analysisModular formsymbolsOrder (ring theory)Moduli spaceNuclear Physics B
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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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An intrinsic characterization of 2+2 warped spacetimes

2010

We give several equivalent conditions that characterize the 2+2 warped spacetimes: imposing the existence of a Killing-Yano tensor $A$ subject to complementary algebraic restrictions; in terms of the projector $v$ (or of the canonical 2-form $U$) associated with the 2-planes of the warped product. These planes are principal planes of the Weyl and/or Ricci tensors and can be explicitly obtained from them. Therefore, we obtain the necessary and sufficient (local) conditions for a metric tensor to be a 2+2 warped product. These conditions exclusively involve explicit concomitants of the Riemann tensor. We present a similar analysis for the conformally 2+2 product spacetimes and give an invaria…

PhysicsPure mathematicsRiemann curvature tensorPhysics and Astronomy (miscellaneous)Degenerate energy levelsFOS: Physical sciencesProduct metricGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointGeneral Relativity and Quantum Cosmologylaw.inventionsymbols.namesakeProjectorlawsymbolsTensorAlgebraic numberInvariant (mathematics)
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An intrinsic characterization of spherically symmetric spacetimes

2010

We give the necessary and sufficient (local) conditions for a metric tensor to be a non conformally flat spherically symmetric solution. These conditions exclusively involve explicit concomitants of the Riemann tensor. As a direct application we obtain the {\em ideal} labeling of the Schwarzschild, Reissner-Nordstr\"om and Lema\^itre-Tolman-Bondi solutions.

PhysicsRiemann curvature tensorIdeal (set theory)Physics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)General Relativity and Quantum CosmologyPhysics::History of PhysicsGeneral Relativity and Quantum Cosmologysymbols.namesakesymbolsSymmetric solutionMetric tensor (general relativity)Schwarzschild radiusMathematical physicsClassical and Quantum Gravity
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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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An intrinsic characterization of the Kerr metric

2009

We give the necessary and sufficient (local) conditions for a metric tensor to be the Kerr solution. These conditions exclusively involve explicit concomitants of the Riemann tensor.

PhysicsRiemann curvature tensorsymbols.namesakePhysics and Astronomy (miscellaneous)Kerr metricsymbolsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)Metric tensor (general relativity)General Relativity and Quantum CosmologyMathematical physics
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An Exact Riemann Solver for Multidimensional Special Relativistic Hydrodynamics

2001

We have generalised the exact solution of the Riemann problem in special relativistic hydrodynamics (Marti and Muller, 1994) for arbitrary tangential flow velocities. The solution is obtained by solving the jump conditions across shocks plus an ordinary differential equation arising from the self-similarity condition along rarefaction waves, in a similar way as in purely normal flow. This solution has been used to build up an exact Riemann solver implemented in a multidimensional relativistic (Godunov-type) hydro-code.

PhysicsRoe solverShock wavesymbols.namesakeRiemann problemExact solutions in general relativityOrdinary differential equationMathematical analysissymbolsJumpAstrophysicsRiemann's differential equationRiemann solver
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