Search results for "Vector"

showing 10 items of 2660 documents

Laser heterodyne displacement measuring using PLZT frequency shifter

1991

Abstract The implementation of a frequency shifter based on lead lanthanum zirconate titanate ceramic (PLZT) and a voltage-controlled λ/4 plate is described. The capabilities of these elements are demonstrated with results from a Michelson-type laser heterodyne displacement measuring interferometer with 0.01 μm accuracy and 1 Hz display update rate.

HeterodyneMaterials sciencebusiness.industryMetals and AlloysLanthanum zirconateCondensed Matter PhysicsLaserTitanateDisplacement (vector)Surfaces Coatings and FilmsElectronic Optical and Magnetic Materialslaw.inventionInterferometryOpticslawvisual_artvisual_art.visual_art_mediumFrequency shifterCeramicElectrical and Electronic EngineeringbusinessInstrumentationSensors and Actuators A: Physical
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Constant circulation sequences of binary neutron stars and their spin characterization

2018

For isentropic fluids, dynamical evolution of a binary system conserves the baryonic mass and circulation; therefore, sequences of constant rest mass and constant circulation are of particular importance. In this work, we present the extension of our Compact Object CALculator (\cocal{}) code to compute such quasiequilibria and compare them with the well-known corotating and irrotational sequences, the latter being the simplest, zero-circulation case. The circulation as a measure of the spin for a neutron star in a binary system has the advantage of being exactly calculable since it is a local quantity. To assess the different measures of spin, such as the angular velocity of the star, the q…

High Energy Astrophysical Phenomena (astro-ph.HE)AstrofísicaPhysics010308 nuclear & particles physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Compact starConservative vector field01 natural sciencesGeneral Relativity and Quantum CosmologyNeutron starCirculation (fluid dynamics)0103 physical sciencesAstronomiaBinary systemConstant (mathematics)Astrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsMathematical physicsDimensionless quantitySpin-½
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Jet launching from binary black hole-neutron star mergers: Dependence on black hole spin, binary mass ratio and magnetic field orientation

2018

Black hole-neutron star (BHNS) mergers are one of the most promising targets for multimessenger astronomy. Using general relativistic magnetohydrodynamic simulations of BHNS undergoing merger we showed that a magnetically--driven jet can be launched by the remnant if the NS is endowed with a dipole B field extending from the interior into the exterior as in a radio pulsar. These self-consistent studies considered a BHNS system with mass ratio $q=3:1$, BH spin $a/M_{BH}=0.75$ aligned with the total orbital angular momentum (OAM), and a NS that is irrotational, threaded by an aligned B field, and modeled by an $\Gamma$--law equation of state with $\Gamma=2$. Here, as a crucial step in establi…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrofísica010308 nuclear & particles physicsEquation of state (cosmology)Star (game theory)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Mass ratioConservative vector field01 natural sciencesGeneral Relativity and Quantum CosmologyOrientation (vector space)Black holeNeutron star0103 physical sciencesAtomic physicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSpin-½
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Striped Blandford/Znajek jets from advection of small-scale magnetic field

2020

Black hole - accretion disc systems are the central engines of relativistic jets from stellar to galactic scales. We numerically quantify the unsteady outgoing Poynting flux through the horizon of a rapidly spinning black hole endowed with a rotating accretion disc. The disc supports small-scale, concentric, flux tubes with zero net magnetic flux. Our General Relativistic force-free electrodynamics simulations follow the accretion onto the black hole over several hundred dynamical timescales in 3D. For the case of counter-rotating accretion discs, the average process efficiency reaches up to $\left\langle\epsilon\right\rangle\approx 0.43$, compared to a stationary energy extraction by the B…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSupermassive black holeField lineAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsMagnetic fluxAccretion (astrophysics)Magnetic fieldBlack holeAstrophysical jetSpace and Planetary SciencePoynting vectorAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaMonthly Notices of the Royal Astronomical Society
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Scalar, axial-vector, and tensor resonances from the rho D-*, omega D-* interaction in the hidden gauge formalism

2009

13 pages, 15 figures.-- PACS nrs.: 13.75.Lb, 12.40.Vv, 12.40.Yx, 14.40.Cs.-- ArXiv pre-print available at: http://arxiv.org/abs/0903.3823

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)[PACS] Meson-meson interactions (energy ≤ 10 GeV)[PACS] Vector-meson dominanceHigh Energy Physics::Phenomenology0202 electrical engineering electronic engineering information engineeringFOS: Physical sciences[PACS] Other mesons with S=C=0 mass < 2.5 GeVFísica020206 networking & telecommunications020201 artificial intelligence & image processing02 engineering and technology[PACS] Hadron mass models and calculations
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Scalar contributions to b→c(u)τν transitions

2017

Abstract We perform a comprehensive analysis of scalar contributions in b → c τ ν transitions including the latest measurements of R ( D ( ⁎ ) ) , the q 2 differential distributions in B → D ( ⁎ ) τ ν , the τ polarization asymmetry for B → D ⁎ τ ν , and the bound derived from the total width of the B c meson. We find that scalar contributions with the simultaneous presence of both left- and right-handed couplings to quarks can explain the available data, specifically R ( D ( ⁎ ) ) together with the measured differential distributions. However, the constraints from the total B c width present a slight tension with the current data on B → D ⁎ τ ν in this scenario, preferring smaller values fo…

High Energy Physics - Phenomenology; High Energy Physics - Phenomenology; High Energy Physics - Experiment; Nuclear and High Energy PhysicsQuarkPhysicsNuclear and High Energy PhysicsParticle physicsMeson010308 nuclear & particles physicsPhysics beyond the Standard Modelmedia_common.quotation_subjectObservablePolarization (waves)01 natural sciences7. Clean energyAsymmetrylcsh:QC1-999High Energy Physics - ExperimentBaryonHigh Energy Physics - Phenomenology0103 physical sciencesCurrent vector010306 general physicslcsh:Physicsmedia_commonPhysics Letters B
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Two-twistor particle models and free massive higher spin fields

2015

We present D=3 and D=4 models for massive particles moving in a new type of enlarged spacetime, with D-1 additional vector coordinates, which after quantization lead to the towers of massive higher spin (HS) free fields. Two classically equivalent formulations are presented: one with a hybrid spacetime/bispinor geometry and a second described by a free two-twistor dynamics with constraints. After quantization in the D=3 and D=4 cases, the wave functions are given as functions on the SL(2,R) and SL(2,C) group manifolds respectively, and describe arbitrary on-shell momenta and spin degrees of freedom. Finally, the D=6 case and possible supersymmetric extensions are mentioned.

High Energy Physics - TheoryBispinorPhysicsNuclear and High Energy PhysicsSpacetimeCoordinate vectorFOS: Physical sciencesMathematical Physics (math-ph)First quantizationSupersymmetryTwistor theoryAdS/CFT correspondenceQuantization (physics)Classical mechanicsHigh Energy Physics - Theory (hep-th)Mathematical PhysicsMathematical physicsJournal of High Energy Physics
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The damped harmonic oscillator in deformation quantization

2005

We propose a new approach to the quantization of the damped harmonic oscillator in the framework of deformation quantization. The quantization is performed in the Schr\"{o}dinger picture by a star-product induced by a modified "Poisson bracket". We determine the eigenstates in the damped regime and compute the transition probability between states of the undamped harmonic oscillator after the system was submitted to dissipation.

High Energy Physics - TheoryDeformation quantization[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]Canonical quantizationGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Poisson bracket[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]Quantum mechanics0103 physical sciencesdissipative systems010306 general physicsNonlinear Sciences::Pattern Formation and Solitonsquantum mechanics.Harmonic oscillatorEigenvalues and eigenvectorsPhysicsQuantum Physics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Quantization (signal processing)quantum mechanicsPACS numbers: 03.50.-z 03.50.De 11.10.-z 03.65.DbLandau quantization16. Peace & justiceSecond quantizationClassical mechanicsHigh Energy Physics - Theory (hep-th)Schrödinger pictureQuantum Physics (quant-ph)
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The Schouten - Nijenhuis bracket, cohomology and generalized Poisson structures

1996

Newly introduced generalized Poisson structures based on suitable skew-symmetric contravariant tensors of even order are discussed in terms of the Schouten-Nijenhuis bracket. The associated `Jacobi identities' are expressed as conditions on these tensors, the cohomological contents of which is given. In particular, we determine the linear generalized Poisson structures which can be constructed on the dual spaces of simple Lie algebras.

High Energy Physics - TheoryMathematics - Differential GeometryPhysicsPure mathematicsSchouten–Nijenhuis bracketFOS: Physical sciencesGeneral Physics and AstronomyOrder (ring theory)Statistical and Nonlinear PhysicsPoisson distributionCohomologysymbols.namesakeBracket (mathematics)High Energy Physics - Theory (hep-th)Differential Geometry (math.DG)Simple (abstract algebra)Mathematics - Quantum AlgebraLie algebraFOS: MathematicssymbolsCovariance and contravariance of vectorsQuantum Algebra (math.QA)Mathematics::Symplectic GeometryMathematical PhysicsJournal of Physics A: Mathematical and General
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Matter dependence of the four-loop QCD cusp anomalous dimension: from small angles to all angles

2019

We compute the fermionic contributions to the cusp anomalous dimension in QCD at four loops as an expansion for small cusp angle. As a byproduct we also obtain the respective terms of the four-loop HQET wave function anomalous dimension. Our new results at small angles provide stringent tests of a recent conjecture for the exact angle dependence of the matter terms in the four-loop cusp anomalous dimension. We find that the conjecture does not hold for two of the seven fermionic color structures, but passes all tests for the remaining terms. This provides strong support for the validity of the corresponding conjectured expressions with full angle dependence. Taking the limit of large Minkow…

High Energy Physics - TheoryNuclear and High Energy PhysicsConformal anomalyFOS: Physical sciencesConformal map01 natural sciencesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Dimension (vector space)Perturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityScattering Amplitudes010306 general physicsWave functionQuantum chromodynamicsCusp (singularity)Physics010308 nuclear & particles physicsPerturbative QCDEffective Field TheoriesWilson ’t Hooft and Polyakov loopsScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Journal of High Energy Physics
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