Search results for "Anisotropy"

showing 10 items of 912 documents

Cosmic microwave background anisotropy: deviations from Gaussianity caused by non-linear gravity

2002

Non-linear evolution of cosmological energy density fluctuations triggers deviations from Gaussianity in the temperature distribution of the cosmic microwave background. A method to estimate these deviations is proposed. N-body simulations - in aCDM cosmology - are used to simulate the strongly non-linear evolution of cosmological structures. It is proved that these simulations can be combined with the potential approximation to calculate the statistical moments of the CMB anisotropies produced by non-linear gravity. Some of these moments are computed and the resulting values are different from those corresponding to Gaussianity.

PhysicsGravity (chemistry)Cosmic microwave backgroundAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmologyGeneral Relativity and Quantum CosmologyNonlinear systemDistribution (mathematics)Space and Planetary ScienceEnergy densityStatistical physicsAnisotropyMonthly Notices of the Royal Astronomical Society
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Great Attractor-like structures and large-scale anisotropy

1994

PhysicsGreat AttractorClassical mechanicsScale (ratio)Space and Planetary ScienceAstronomy and AstrophysicsStatistical physicsAnisotropyMonthly Notices of the Royal Astronomical Society
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Improving on numerical simulations of nonlinear CMB anisotropies

2015

An Adaptative-Particle-Particle-Particle-Mesh code (HYDRA) plus a ray-tracing procedure was used in [1] to perform an exhaustive analysis of the weak lensing anisotropy. Other nonlinear Cosmic Microwave Background anisotropies, such as the Rees-Sciamaand the Sunyaev-Zel.dovicheffects are also being studied by using the same tools. Here we present some advances in our study of these nonlinear anisotropies. The primary advance is due to the use of better simulations with greater particle densities and appropriate softening, although other parameters have also been adjusted to get better estimates. Thus, we improve on a previous paper [2] where the Rees-Sciamaeffect was studied with Particle-M…

PhysicsHistoryNonlinear systemCosmic microwave backgroundResolution improvementAstrophysics::Cosmology and Extragalactic AstrophysicsStatistical physicsFocus (optics)AnisotropySofteningWeak gravitational lensingComputer Science ApplicationsEducationJournal of Physics: Conference Series
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A general approach for the calculation of the energy levels and the inelastic neutron scattering cross-section of highly nuclear magnetic clusters

1997

Abstract We develop here a general approach to calculate in an efficient way the spin levels as well as the spin eigenfunctions and the INS intensities of clusters formed by large numbers of exchange-coupled magnetic metal ions. The approach is based on the successive use of the irreducible tensor operator techniques and takes into account all kinds of magnetic exchange interactions between the metal ions. The potentialities of this approach are illustrated from an example comprising nine exchange-coupled Ni (II) ions.

PhysicsInelastic scatteringEigenfunctionCondensed Matter PhysicsInelastic neutron scatteringElectronic Optical and Magnetic MaterialsIonCross section (physics)Magnetic anisotropyCondensed Matter::Strongly Correlated ElectronsElectrical and Electronic EngineeringAtomic physicsTensor operatorSpin-½Physica B: Condensed Matter
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Resummation of anisotropic quartic oscillator. Crossover from anisotropic to isotropic large-order behavior

1996

We present an approximative calculation of the ground-state energy for the anisotropic anharmonic oscillator Using an instanton solution of the isotropic action $\delta = 0$, we obtain the imaginary part of the ground-state energy for small negative $g$ as a series expansion in the anisotropy parameter $\delta$. From this, the large-order behavior of the $g$-expansions accompanying each power of $\delta$ are obtained by means of a dispersion relation in $g$. These $g$-expansions are summed by a Borel transformation, yielding an approximation to the ground-state energy for the region near the isotropic limit. This approximation is found to be excellent in a rather wide region of $\delta$ aro…

PhysicsInstantonQuantum PhysicsIsotropyFOS: Physical sciencesAtomic and Molecular Physics and OpticsQuartic functionDispersion relationQuantum electrodynamicsLimit (mathematics)ResummationAnisotropySeries expansionQuantum Physics (quant-ph)
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Black hole accretion discs and jets at super-Eddington luminosity

2005

Super-Eddington accretion discs with 3 and 15 dot M_E around black holes with mass 10 M_sun are examined by two-dimensional radiation hydrodynamical calculations extending from the inner disc edge to 5*10^4 r_g and lasting up to \sim 10^6 r_g/c. The dominant radiation-pressure force in the inner region of the disc accelerates the gas vertically to the disc plane, and jets with 0.2 -- 0.4$c$ are formed along the rotational axis. In the case of the lower accretion rate, the initially anisotropic high-velocity jet expands outward and becomes gradually isotropic flow in the distant region. The mass-outflow rate from the outer boundary is as large as \sim 10^{19} -- 10^{23} g s^{-1}, but it is v…

PhysicsJet (fluid)Accretion (meteorology)Degree (graph theory)Plane (geometry)Astrophysics::High Energy Astrophysical PhenomenaAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLuminosityBlack holesymbols.namesakeSpace and Planetary ScienceEddington luminositysymbolsAnisotropyAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Vectorial Kerr-cavity solitons.

2000

It is shown that a Kerr cavity with different losses for the two polarization components of the field can support both dark and bright cavity solitons (CS’s). A parametrically driven Ginzburg–Landau equation is shown to describe the system for large-cavity anisotropy. In one transverse dimension the nonlinear dynamics of the bright CS’s is numerically investigated.

PhysicsKerr effectbusiness.industryNumerical analysisPhysics::OpticsAstrophysics::Cosmology and Extragalactic AstrophysicsPolarization (waves)Atomic and Molecular Physics and OpticsNonlinear systemOpticsLight propagationPhysics::Accelerator PhysicsTransverse dimensionbusinessAnisotropyNonlinear Sciences::Pattern Formation and SolitonsOptics letters
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Higher Harmonic Anisotropic Flow Measurements of Charged Particles in Pb-Pb Collisions atsNN=2.76  TeV

2011

We report on the first measurement of the triangular nu(3), quadrangular nu(4), and pentagonal nu(5) charged particle flow in Pb-Pb collisions at root s(NN) = 2.76 TeV measured with the ALICE detector at the CERN Large Hadron Collider. We show that the triangular flow can be described in terms of the initial spatial anisotropy and its fluctuations, which provides strong constraints on its origin. In the most central events, where the elliptic flow nu(2) and nu(3) have similar magnitude, a double peaked structure in the two-particle azimuthal correlations is observed, which is often interpreted as a Mach cone response to fast partons. We show that this structure can be naturally explained fr…

PhysicsLarge Hadron Collider010308 nuclear & particles physicsElliptic flowGeneral Physics and AstronomyParton01 natural sciencesCharged particleNuclear physicssymbols.namesakeFlow (mathematics)Mach number0103 physical sciencessymbolsHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsAnisotropyFourier seriesPhysical Review Letters
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Measurements of mass-dependent azimuthal anisotropy in central p + Au, d + Au, and He3 + Au collisions at sNN=200 GeV

2018

We present measurements of the transverse- momentum dependence of elliptic flow v2 for identified pions and (anti)protons at midrapidity (|η|<0.35), in 0%–5% central p+Au and He3+Au collisions at sNN=200 GeV. When taken together with previously published measurements in d+Au collisions at sNN=200 GeV, the results cover a broad range of small-collision-system multiplicities and intrinsic initial geometries. We observe a clear mass-dependent splitting of v2(pT) in d+Au and He3+Au collisions, just as in large nucleus-nucleus (A+A) collisions, and a smaller splitting in p+Au collisions. Both hydrodynamic and transport model calculations successfully describe the data at low pT (<1.5GeV/c), but …

PhysicsLarge Hadron Collider010308 nuclear & particles physicsNuclear TheoryHadronElliptic flowConstituent quarkMultiplicity (mathematics)Kinetic energy01 natural sciencesNuclear physicsPion0103 physical sciencesNuclear Experiment010306 general physicsAnisotropyPhysical Review C
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Measurement of the suppression and azimuthal anisotropy of muons from heavy-flavor decays in Pb+Pb collisions at sNN=2.76 TeV with the ATLAS detector

2018

ATLAS measurements of the production of muons from heavy-flavor decays in root s(NN) = 2.76 TeV Pb+Pb collisions and root s = 2.76 TeV pp collisions at the LHC are presented. Integrated luminositie ...

PhysicsLarge Hadron ColliderMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAtlas detectorHigh Energy Physics::PhenomenologyHadron01 natural sciencesAzimuthNuclear physicsmedicine.anatomical_structureAtlas (anatomy)0103 physical sciencesmedicinePhysics::Accelerator PhysicsHigh Energy Physics::ExperimentAngular dependenceNuclear Experiment010306 general physicsAnisotropyPhysical Review C
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