Search results for "ROTATIONAL"

showing 10 items of 381 documents

Simulations of an inhomogeneous stellar wind interacting with a pulsar wind in a binary system

2014

Binary systems containing a massive star and a non-accreting pulsar present strong interaction between the stellar and the pulsar winds. The properties of this interaction, which largely determine the non-thermal radiation in these systems, strongly depend on the structure of the stellar wind, which can be clumpy or strongly anisotropic, as in Be stars. We study numerically the influence of inhomogeneities in the stellar wind on the structure of the two-wind interaction region. We carried out for the first time axisymmetric, relativistic hydrodynamical simulations, with Lorentz factors of ~6 and accounting for the impact of instabilities, to study the impact in the two-wind interaction stru…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::High Energy Astrophysical PhenomenaLorentz transformationStrong interactionRotational symmetryFOS: Physical sciencesBinary numberAstronomy and AstrophysicsContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakePulsar13. Climate actionSpace and Planetary SciencePhysics::Space PhysicssymbolsAstrophysics::Solar and Stellar AstrophysicsDensity contrastAstrophysics - High Energy Astrophysical PhenomenaAnisotropyPhysics::Atmospheric and Oceanic PhysicsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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Magnetorotational Instability in Core-Collapse Supernovae

2017

We discuss the relevance of the magnetorotational instability (MRI) in core-collapse supernovae (CCSNe). Our recent numerical studies show that in CCSNe, the MRI is terminated by parasitic instabilities of the Kelvin-Helmholtz type. To determine whether the MRI can amplify initially weak magnetic fields to dynamically relevant strengths in CCSNe, we performed three-dimensional simulations of a region close to the surface of a differentially rotating proto-neutron star in non-ideal magnetohydrodynamics with two different numerical codes. We find that under the conditions prevailing in proto-neutron stars, the MRI can amplify the magnetic field by (only) one order of magnitude. This severely …

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsFOS: Physical sciencesGeneral Physics and AstronomyCollapse (topology)AstrophysicsMagnetic fieldCore (optical fiber)StarsSupernovaAstrophysics - Solar and Stellar AstrophysicsMagnetorotational instabilityMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaSolar and Stellar Astrophysics (astro-ph.SR)Order of magnitudeActa Physica Polonica B Proceedings Supplement
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Propagation and stability of relativistic jets

2020

A simple look at the steady high-energy Universe reveals a clear correlation with outflows generated around compact objects (winds and jets). In the case of relativistic jets, they are thought to be produced as a consequence of the extraction of rotational energy from a Kerr black hole (Blandford-Znajek), or from the disc (Blandford-Payne). A fraction of the large energy budget provided by accretion and/or black hole rotational energy is invested into jet formation. After formation, the acceleration and collimation of these outflows allow them to propagate to large distances away from the compact object. The synchrotron cooling times demand that re-acceleration of particles takes place alon…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Radio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCompact starRotational energyBlack holeParticle accelerationRotating black holeAstrophysical jetAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy AstrophysicsProceedings of High Energy Phenomena in Relativistic Outflows VII — PoS(HEPRO VII)
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Low-temperature microwave response of heavy-fermion compounds

2009

The electrodynamic properties of heavy fermions are distinct from those of normal metals due to the reduced transport relaxation rate that goes hand in hand with the enhanced mass. Using broadband microwave spectroscopy on thin-film samples of the heavy-fermion materials UPd2Al3 and UNi2Al3, we find that the frequency-dependent conductivity of these compounds at low temperatures follows a simple Drude prediction. The observed relaxation rates in the GHz frequency range are extremely low for a metal.

HistoryRange (particle radiation)Materials scienceCondensed matter physicsRelaxation rateHeavy fermionMicrowave responseRelaxation (physics)Rotational spectroscopyFermionConductivityComputer Science ApplicationsEducationJournal of Physics: Conference Series
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Determination of concentrations in ternary and quaternary molecular gas mixtures using femtosecond Raman spectroscopy

2002

European Conference on Nonlinear Optical Spectroscopy MAR 18-19, 2002 VILLIGEN, SWITZERLAND; Measurements of concentrations in gas mixtures of three and four molecular components are presented. They rely on a femtosecond time-resolved pump-probe technique based on Raman-induced polarization spectroscopy. The rotational time response of the molecular gas mixture is measured as a function of the pump-probe time delay. No selective frequency tunability is needed as the molecular rotational spectra are excited within the laser bandwidth. The results obtained from experiments performed at room temperature in N2O-CO2-N2 and N2O-CO2-O2-N2 mixtures are presented and the accuracy of the method is di…

INDUCED POLARIZATION SPECTROSCOPYCO2Q-BRANCHROTATIONAL COHERENCEBAND
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Line mixing in the ν1 and 2ν2 isotropic Raman Q-branch of CO2 perturbed by argon and helium

1999

0021-9606; The shapes of the ν1 and 2ν2 isotropic Raman Q-branch of CO2 perturbed by argon and helium have been measured by Stimulated Raman Spectroscopy (SRS) or coherent anti-Stokes Raman Spectroscopy (CARS) techniques. The data have been successfully analyzed with an energy corrected sudden (ECS) approximation model based on basic rates determined independently. Finally comparison of the present data with time resolved double resonance experiments allows us to discuss the physical origin of the two empirical constants which account for the shift and broadening of the branch due to vibrational effects. (C) 1999 American Institute of Physics. [S0021-9606(99)00344-X].

INFRARED-SPECTRA1000SPECTROSCOPYGASFERMI DYADDOUBLE-RESONANCE EXPERIMENTSROTATIONAL ENERGY-TRANSFERVIBRATIONAL-RELAXATIONPRESSURENU-1/2-NU-2BAND SHAPESBAR
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Concentration measurements in molecular gas mixtures with a two-pump pulse femtosecond polarization spectroscopy technique

2001

0021-9606; Recently, we have demonstrated the ability of the Raman-induced polarization spectroscopy (RIPS) technique to accurately determine concentration or polarizability anisotropy ratio in low-pressure binary molecular mixtures [E. Hertz, B. Lavorel, O. Faucher, and R. Chaux, J. Chem. Phys. 113, 6629 (2000)]. It has been also pointed out that macroscopic interference, occurring when two revivals associated to different molecules time overlap, can be used to achieve measurements with picosecond time resolution. The applicability of the technique is intrinsically limited to a concentration range where the signals of both molecules are of the same magnitude. In this paper, a two-pump puls…

INTERFERENCEDYNAMICS010304 chemical physicsChemistrybusiness.industryGeneral Physics and AstronomyPulse sequenceTRANSITIONSPolarization (waves)01 natural sciencesMolecular physicsROTATIONAL COHERENCEOpticsPolarizabilityPicosecond0103 physical sciencesFemtosecondCO2Physical and Theoretical ChemistryTime-resolved spectroscopy010306 general physicsSpectroscopyAnisotropybusinessPOPULATION
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ROTATIONAL TOLERANCES IN ABUTMENT-IMPLANT CONNECTION FOR ORIGINAL AND COMPATIBLE ABUTMENTS

2022

Implant Abutment Connection Rotational tolerances
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Equilibrium geometries of cyclic SiC3 isomers

2001

Equilibrium geometries of two isomers of cyclic SiC3 are determined by both large scale ab initio calculation and a procedure involving the use of experimental data from microwave spectroscopy and calculated harmonic and cubic force fields. Internuclear distances corresponding to structures obtained by both procedures agree to better than 0.003 A in all cases, allowing for precise recommendations of equilibrium structures. Rather large residual inertial defects obtained from moments of inertia based on rotational constants adjusted for effects of vibration–rotation interaction were found to be reduced significantly by inclusion of electronic contributions as estimated from calculations of r…

Inertial frame of referenceClassical mechanicsScale (ratio)ChemistryAb initio quantum chemistry methodsAb initioGeneral Physics and AstronomyHarmonic (mathematics)Rotational spectroscopyPhysical and Theoretical ChemistryMoment of inertiaResidualMolecular physicsThe Journal of Chemical Physics
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Cyclic SiS2: a new perspective on the Walsh rules.

2012

Information retrievalChemistryComputational chemistryPerspective (graphical)General ChemistryRotational spectroscopyCatalysisAngewandte Chemie (International ed. in English)
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