Search results for "singularity."

showing 10 items of 346 documents

On numerical relativistic hydrodynamics and barotropic equations of state

2012

The characteristic formulation of the relativistic hydrodynamic equations (Donat et al 1998 J. Comput. Phys. 146 58), which has been implemented in many relativistic hydro-codes that make use of Godunov-type methods, has to be slightly modified in the case of evolving barotropic flows. For a barotropic equation of state, a removable singularity appears in one of the eigenvectors. The singularity can be avoided by means of a simple renormalization which makes the system of eigenvectors well defined and complete. An alternative strategy for the particular case of barotropic flows is discussed.

PhysicsEquation of statePhysics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyRenormalizationClassical mechanicsSingularityAstrophysics - Solar and Stellar AstrophysicsSimple (abstract algebra)Barotropic fluidSolar and Stellar Astrophysics (astro-ph.SR)Eigenvalues and eigenvectorsAlternative strategyRemovable singularityClassical and Quantum Gravity
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Feynman graph polynomials

2010

The integrand of any multi-loop integral is characterised after Feynman parametrisation by two polynomials. In this review we summarise the properties of these polynomials. Topics covered in this article include among others: Spanning trees and spanning forests, the all-minors matrix-tree theorem, recursion relations due to contraction and deletion of edges, Dodgson's identity and matroids.

PhysicsFeynman parametrizationNuclear and High Energy PhysicsSpanning treeFOS: Physical sciencesAstronomy and AstrophysicsGraph theoryMathematical Physics (math-ph)Symbolic computationMatroidLoop integralAtomic and Molecular Physics and OpticsCombinatoricsHigh Energy Physics - PhenomenologySingularityHigh Energy Physics - Phenomenology (hep-ph)Contraction (operator theory)Mathematical Physics
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Relating the finite-volume spectrum and the two-and-three-particle S matrix for relativistic systems of identical scalar particles

2017

Working in relativistic quantum field theory, we derive the quantization condition satisfied by coupled two- and three-particle systems of identical scalar particles confined to a cubic spatial volume with periodicity $L$. This gives the relation between the finite-volume spectrum and the infinite-volume $\textbf 2 \to \textbf 2$, $\textbf 2 \to \textbf 3$ and $\textbf 3 \to \textbf 3$ scattering amplitudes for such theories. The result holds for relativistic systems composed of scalar particles with nonzero mass $m$, whose center of mass energy lies below the four-particle threshold, and for which the two-particle $K$ matrix has no singularities below the three-particle threshold. The quan…

PhysicsFinite volume methodNuclear Theory010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciences01 natural sciencesNuclear Theory (nucl-th)Scattering amplitudeQuantization (physics)High Energy Physics - LatticeQuantum mechanics0103 physical sciencesGravitational singularityBoundary value problemQuantum field theory010306 general physicsNuclear theoryS-matrixPhysical Review D
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Analysis of high-harmonic generation in terms of complex Floquet spectral analysis

2017

Recent developments on intense laser sources is opening a new field of optical sciences. An intense coherent light beam strongly interacting with the matter causes a coherent motion of a particle, forming a strongly dressed excited particle. A photon emission from this dressed excited particle is a strong nonlinear process causing high-harmonic generation (HHG), where the perturbation analysis is broken down. In this work, we study a coherent photon emission from a strongly dressed excited atom in terms of complex spectral analysis in the extended Floquet-Hilbert-space. We have obtained the eigenstates of the total Hamiltonian with use of Feshbach-Brilloiun-Wigner projection method. In this…

PhysicsFloquet theoryQuantum PhysicsPhotonElectromagneticsFloquet spectral analysisTime evolutionFOS: Physical sciencesHigh harmonic generationsymbols.namesakeSingularityExcited statesymbolsHigh harmonic generationPhysics::Atomic PhysicsAtomic physicsHamiltonian (quantum mechanics)Quantum Physics (quant-ph)Physics - OpticsOptics (physics.optics)
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Multifractal wave functions at the Anderson transition.

1991

Electronic wave functions in disordered systems are studied within the Anderson model of localization. At the critical disorder in 3D we diagonalize very large (103 823\ifmmode\times\else\texttimes\fi{}103 823) secular matrices by means of the Lanczos algorithm. On all length scales the obtained strong spatial fluctuations of the amplitude of the eigenstates display a multifractal character, reflected in the set of generalized fractal dimensions and the singularity spectrum of the fractal measure. An analysis of 1D systems shows multifractality too, in contrast to previous claims.

PhysicsFractalAmplitudeGeneral Physics and AstronomyLanczos algorithmMultifractal systemSingularity spectrumWave functionCondensed Matter::Disordered Systems and Neural NetworksAnderson impurity modelFractal dimensionMathematical physicsPhysical review letters
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Point field models for the galaxy point pattern modelling the singularity of the two-point correlation function

2002

There is empirical evidence that the two-point correlation function of the galaxy distribution follows, for small scales, reasonably well a power-law expression $\xi(r)\propto r^{-\gamma}$ with $\gamma$ between 1.5 and 1.9. Nevertheless, most of the point field models suggested in the literature do not have this property. This paper presents a new class of models, which is produced by modifying point fields commonly used in cosmology to mimic the galaxy distribution, but where $\gamma=2$ is too large. The points are independently and randomly shifted, leading to the desired reduction of the value of $\gamma$.

PhysicsGalaxy statistics ; Large-scale structure of universe ; Statistical methodField (physics)Distribution (number theory)Astrophysics (astro-ph)FOS: Physical sciencesLarge-scale structure of universeAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy statisticsExpression (computer science)UNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]CosmologyGalaxySingularityCorrelation functionSpace and Planetary SciencePoint (geometry)Statistical physicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaStatistical method:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Regularized Euler-alpha motion of an infinite array of vortex sheets

2016

We consider the Euler- $$\alpha $$ regularization of the Birkhoff–Rott equation and compare its solutions with the dynamics of the non regularized vortex-sheet. For a flow induced by an infinite array of planar vortex-sheets we analyze the complex singularities of the solutions.Through the singularity tracking method we show that the regularized solution has several complex singularities that approach the real axis. We relate their presence to the formation of two high-curvature points in the vortex sheet during the roll-up phenomenon.

PhysicsGeneral Mathematics010102 general mathematicsMathematical analysisGeometryVortex-sheet Birkhoff–Rott equation Euler-alpha regularization Complex singularities01 natural sciencesRegularization (mathematics)010305 fluids & plasmasVortexsymbols.namesakeSingularityFlow (mathematics)0103 physical sciencesVortex sheetEuler's formulasymbolsGravitational singularity0101 mathematicsComplex planeSettore MAT/07 - Fisica Matematica
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The Palatini Approach Beyond Einstein’s Gravity

2014

I review recent results obtained for extensions of general relativity formulated within the Palatini formalism, an approach in which metric and connection are treated as independent geometrical entities. The peculiar dynamics of these theories, governed by second-order equations and having no new degrees of freedom, makes them specially suitable to address certain aspects of quantum gravity phenomenology, construct nonsingular bouncing cosmologies, and explore black hole interiors, which in the Reissner-Nordstrom case develop a compact core of finite density instead of a point-like singularity.

PhysicsGeneral relativityBlack starlaw.inventionGeneral Relativity and Quantum Cosmologysymbols.namesakeSingularityInvertible matrixClassical mechanicslawsymbolsQuantum gravityEinsteinPhenomenology (particle physics)Ring singularity
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Geons in Palatini Theories of Gravity

2017

An explicit implementation of geons in the context of gravitational theories extending general relativity is discussed in detail. Such extensions are formulated in the Palatini approach, where metric and affine connection are regarded as independent entities. This formulation is inspired on the macroscopic description of the physics of crystalline structures with defects in the context of solid-state physics, whose study can provide valuable lessons for going beyond GR. We discuss several theories for the gravitational field including additional contributions of the Ricci tensor in four and higher dimensions. As opposed to the standard metric approach, the Palatini formulation generates gho…

PhysicsGeodesics in general relativitySpacetime010308 nuclear & particles physicsGeneral relativity01 natural sciencesGravitationGeneral Relativity and Quantum CosmologyClassical mechanicsGravitational field0103 physical sciencesGravitational singularityWormhole010306 general physicsGeon (physics)
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Cosmic censorship conjecture in some matching spherical collapsing metrics

2017

A physically plausible Lema{\^{\i}}tre-Tolman-Bondi collapse in the marginally bound case is considered. By "physically plausible" we mean that the corresponding metric is ${\cal C}^1$ matched at the collapsing star surface and further that its {\em intrinsic} energy is, as due, stationary and finite. It is proved for this Lema{\^{\i}}tre-Tolman-Bondi collapse, for some parameter values, that its intrinsic central singularity is globally naked, thus violating the cosmic censorship conjecture with, for each direction, one photon, or perhaps a pencil of photons, leaving the singularity and reaching the null infinity. Our result is discussed in relation to some other cases in the current liter…

PhysicsGravitacióConjecture010308 nuclear & particles physicsStar (game theory)media_common.quotation_subjectCosmic censorship hypothesisNull (mathematics)Collapse (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsInfinity01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologySingularityRelativitat general (Física)0103 physical sciencesGravitational singularity010306 general physicsMathematical physicsmedia_common
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