Search results for "Core"

showing 10 items of 1999 documents

Observational Effects of Anomalous Boundary Layers in Relativistic Jets

2008

Recent theoretical work has pointed out that the transition layer between a jet an the medium surrounding it may be more complex than previously thought. Under physically realizable conditions, the transverse profile of the Lorentz factor in the boundary layer can be non-monotonic, displaying the absolute maximum where the flow is faster than at the jet spine, followed by an steep fall off. Likewise, the rest-mass density, reaches an absolute minimum (coincident with the maximum in Lorentz factor) and then grows until it reaches the external medium value. Such a behavior is in contrast to the standard monotonic decline of the Lorentz factor (from a maximum value at the jet central spine) an…

PhysicsJet (fluid)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesBoundary (topology)Astronomy and AstrophysicsObservableMechanicsAstrophysicsAstrophysicsCore (optical fiber)Transverse planeBoundary layerLorentz factorsymbols.namesakeAstrophysical jetSpace and Planetary SciencesymbolsThe Astrophysical Journal
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Angular Energy Distribution of Collapsar-Jets

2008

Collapsars are fast-spinning, massive stars, whose core collapse liberates an energy, that can be channeled in the form of ultrarelativistic jets. These jets transport the energy from the collapsed core to large distances, where it is dissipated in the form of long-duration gamma-ray bursts. In this paper we study the dynamics of ultrarelativistic jets produced in collapsars. Also we extrapolate our results to infer the angular energy distribution of the produced outflows in the afterglow phase. Our main focus is to look for global energetical properties which can be imprinted by the different structure of different progenitor stars. Thus, we employ a number of pre-supernova, stellar models…

PhysicsJet (fluid)Shock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRotational energyAfterglowCore (optical fiber)StarsLorentz factorsymbols.namesakeSpace and Planetary SciencesymbolsFree expansionAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Galaxy Astrophysics
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Fine Thermal Structure of a Coronal Active Region

2007

著者人数:12名

PhysicsMultidisciplinaryLine-of-sightbusiness.industryLOOPSCoronal loopCoronaComputational physicsNanoflareslaw.inventionCore (optical fiber)TelescopeOpticslawCoronal planePhysics::Space PhysicsThermalAstrophysics::Solar and Stellar AstrophysicsbusinessX-RAY TELESCOPEScience
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Sn108studied with intermediate-energy Coulomb excitation

2005

The unstable neutron-deficient Sn-108 isotope has been studied in inverse kinematics by intermediate-energy Coulomb excitation using the RISING/FRS experimental setup at GSI. This is the highest Z nucleus studied so far with this method. Its reduced transition probability B (E2;0(g.s.)(+)-> 2(1)(+)) has been measured for the first time. The extracted B(E2) value of 0.230(57)e(2) b(2) has been determined relative to the known value in the stable Sn-112 isotope. The result is discussed in the framework of recent large-scale shell model calculations performed with realistic effective interactions. The roles of particle-hole excitations of the Sn-100 core and of the Z=50 shell gap for the E2 po…

PhysicsNuclear and High Energy PhysicsIsotope010308 nuclear & particles physicsNuclear shell modelShell (structure)Coulomb excitationPolarization (waves)01 natural sciencesCore (optical fiber)medicine.anatomical_structure0103 physical sciencesmedicineNeutronAtomic physicsNuclear Experiment010306 general physicsNucleusPhysical Review C
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Coexistence of triaxial and prolate shapes in 171Ir

1999

Abstract Excited states in 171Ir have been observed for the first time. Gamma-rays were assigned to the nucleus by the recoil-decay tagging method. The ground-state band has a structure consistent with an h 11 2 proton coupled to a core of large triaxial deformation. At high spins, a bandcrossing occurs which is interpreted as a change in shape to a prolate deformation. Band-mixing calculations are performed for 171–175Ir. These show that shape-coexistence between triaxial and prolate states in these nuclei follows the same systematics found in their Pt and Os neighbours. The systematics are also compared with deformations calculated for 171–179Ir using the code “Ultimate Cranker”. Dipole b…

PhysicsNuclear and High Energy PhysicsProtonSpinsNuclear TheoryDeformation (meteorology)RotationCore (optical fiber)Dipolemedicine.anatomical_structureExcited statemedicineAtomic physicsNucleusNuclear Physics A
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Experimental evidence for chirality in the odd-A 105Rh

2004

Abstract High-spin states in 105 Rh were populated by the 96 Zr( 13 C, p3n) reaction at beam energies of 51 and 58 MeV, and studied using the EUROBALL IV γ -ray spectrometer and the DIAMANT charged particle array. A pair of nearly degenerate Δ I = 1 three-quasiparticle bands with the same spins and parity have been observed. Comparison of the experimental results with tilted axis cranking calculations confirms the chiral character of the two bands, while arguments based on the excitation of particles within the π g 9 / 2 ν ( h 11 / 2 ) 2 configuration of the yrast band and comparison with the previously observed γ band exclude the other possible interpretations. This is the first experiment…

PhysicsNuclear and High Energy PhysicsSpins010308 nuclear & particles physics[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]Chiral partner bandsYrastDegenerate energy levelsParity (physics)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Tilted axis cranking01 natural sciences21.10.Re; 21.60.-n; 23.20.Lv; 27.60.+jCore-quasiparticle coupling calculationsCharged particleThree-quasiparticle configuration0103 physical sciencesQuasiparticleAtomic physics010306 general physicsChirality (chemistry)ExcitationPhysics Letters B
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EXTRACTION OF ΛΛ SCATTERING LENGTH

2009

We determine ΛΛ scattering parameters from a ΛΛ invariant mass spectrum that was obtained by 12 C (K-, K+ΛΛ) reaction at the KEK Proton Synchrotron. In the framework of Watson's procedure, the obtained scattering length [Formula: see text] and effective range [Formula: see text] are most consistent with the values predicted by using the Nijmegen soft core models (NSC97's). However, the predicted values by using the Nijmegen hard-core ND ( G -matrix) and the extended soft-core (ESC00) models are out of two standard deviations from the determined scattering parameters.

PhysicsNuclear physicsNuclear and High Energy PhysicsRange (particle radiation)Soft coreExtraction (chemistry)Scattering parametersGeneral Physics and AstronomyProton SynchrotronInvariant massScattering lengthLambdaStandard deviationInternational Journal of Modern Physics E
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The earth Mantle-Core effect in charge-asymmetries for atmospheric neutrino oscillations

2002

Earth medium effects in the three-neutrino oscillations of atmospheric neutrinos are observable under appropriate conditions. This paper generalizes the study of the medium effects and the possibility of their observation in the atmospheric neutrino oscillations from the case of neutrinos traversing only the Earth mantle, where the density is essentially constant, to the case of atmospheric neutrinos crossing also the Earth core. In the latter case new resonance-like effects become apparent. We calculate the CPT-odd asymmetry for the survival probability of muon neutrinos and the observable muon-charge asymmetry, taking into account the different atmospheric neutrino fluxes, and show the de…

PhysicsParticle physicsNuclear and High Energy PhysicsMuonPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFísicaObservableAsymmetryCore (optical fiber)MomentumMagnitude (astronomy)High Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoMixing (physics)media_commonPhysics Letters B
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Towards relativistic simulations of magneto-rotational core collapse

2007

We present a new general relativistic hydrodynamics code specifically designed to study magneto-rotational, relativistic, stellar core collapse. The code is an extension of an existing (and thoroughly tested) hydrodynamics code, which has been applied in the recent past to study relativistic rotational core collapse. It is based on the conformally-flat approximation of Einstein's field equations and conservative formulations for the magneto-hydrodynamics equations. As a first step towards magneto-rotational core collapse simulations the code assumes a passive (test) magnetic field. The paper is focused on the description of the technical details of the numerical implementation, with emphasi…

PhysicsPhysics and Astronomy (miscellaneous)Astrophysics (astro-ph)FOS: Physical sciencesCollapse (topology)General Relativity and Quantum Cosmology (gr-qc)AstrophysicsMechanicsAstrophysicsGeneral Relativity and Quantum CosmologyMagnetic fieldStellar coreCore (optical fiber)symbols.namesakesymbolsCode (cryptography)EinsteinField equationMagneto
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Projections and isolated points of parts of the spectrum

2018

‎‎In this paper‎, ‎we relate the existence of certain projections‎, ‎commuting with a bounded linear operator $T\in L(X)$ acting on Banach space $X$‎, ‎with the generalized Kato decomposition of $T$‎. ‎We also relate the existence of these projections with some properties of the quasi-nilpotent part $H_0(T)$ and the analytic core $K(T)$‎. ‎Further results are given for the isolated points of some parts of the spectrum‎.

PhysicsPure mathematics47A11‎Algebra and Number Theory‎localized SVEP‎‎spectrum‎47A53‎Spectrum (functional analysis)Banach spaceLocalized SVEPKato decompositionBounded operator47A10SpectrumCore (graph theory)Decomposition (computer science)‎47A55Analysis
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