Search results for "Angular"

showing 10 items of 1774 documents

On-Sky Tests of a High-Power Pulsed Laser for Sodium Laser Guide Star Adaptive Optics

2016

We present results of on-sky tests performed in the summer of 2013 to characterize the performance of a prototype high-power pulsed laser for adaptive optics. The laser operates at a pulse repetition rate (PRR) of 600–800[Formula: see text]Hz, with a 6% duty cycle. Its coupling efficiency was found to be, in the best test case (using 18[Formula: see text]W of transmitted power), [Formula: see text] photons s[Formula: see text] sr[Formula: see text] atom[Formula: see text] W[Formula: see text] m2 when circular polarization was employed and [Formula: see text] photons s[Formula: see text] sr[Formula: see text] atom[Formula: see text] W[Formula: see text] m2 with linear polarization. No impro…

PhysicsLinear polarizationbusiness.industryAstronomy and AstrophysicsLaser01 natural scienceslaw.invention010309 opticsLaser guide starOpticsAngular diameterlawDuty cycle0103 physical sciencesLaser power scalingAdaptive opticsbusiness010303 astronomy & astrophysicsInstrumentationCircular polarizationJournal of Astronomical Instrumentation
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Precision measurement of the ratio BR(KS→π+π−e+e−)/BR(KL→π+π−πD0)

2011

Abstract The K S → π + π − e + e − decay mode was investigated using the data collected in 2002 by the NA48/1 Collaboration. With about 23 k K S → π + π − e + e − events and 59 k K L → π + π − π D 0 normalization decays, the K S → π + π − e + e − branching ratio relative to the K L → π + π − π D 0 one was determined to be BR ( K S → π + π − e + e − ) / BR ( K L → π + π − π D 0 ) = ( 3.28 ± 0.06 stat ± 0.04 syst ) × 10 − 2 . This result was used to set the upper limit | g E1 / g BR | 3.0 at 90% CL on the presence, in the decay amplitude, of an E1 direct emission ( g E1 ) term relative to the dominant inner bremsstrahlung ( g BR ) term. The CP-violating asymmetry A ϕ in the sin ϕ cos ϕ distri…

PhysicsNuclear and High Energy PhysicsAngular distribution010308 nuclear & particles physicsBranching fraction0103 physical sciencesBremsstrahlungPiAnalytical chemistryCP violation010306 general physics01 natural sciencesPhysics Letters B
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The Baryon Oscillation Spectroscopic Survey of SDSS-III

2012

The Baryon Oscillation Spectroscopic Survey (BOSS) is designed to measure the scale of baryon acoustic oscillations (BAO) in the clustering of matter over a larger volume than the combined efforts of all previous spectroscopic surveys of large-scale structure. BOSS uses 1.5 million luminous galaxies as faint as i = 19.9 over 10,000 deg(2) to measure BAO to redshifts z < 0.7. Observations of neutral hydrogen in the Ly alpha forest in more than 150,000 quasar spectra (g < 22) will constrain BAO over the redshift range 2.15 < z < 3.5. Early results from BOSS include the first detection of the large-scale three-dimensional clustering of the Ly alpha forest and a strong detection from the Data R…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Settore FIS/05 - Astronomia e AstrofisicaObservacions astronòmiques0103 physical sciencesPhysical Sciences and Mathematicsobservations [Cosmology]010303 astronomy & astrophysicsObservationsAstrophysics::Galaxy AstrophysicsPhysicsCosmologia010308 nuclear & particles physicsAngular diameter distanceAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsQuasarCosmology and Extragalactic AstrophysicsLyman-alpha forestRedshiftGalaxyCosmologyBaryonBossSpace and Planetary ScienceAstronomiaBaryon acoustic oscillationsAstronomical observationsAstrophysics - Cosmology and Nongalactic Astrophysics
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Discrete-Gauss states and the generation of focussing dark beams

2014

Discrete-Gauss states are a new class of gaussian solutions of the free Schr\"odinger equation owning discrete rotational symmetry. They are obtained by acting with a discrete deformation operator onto Laguerre-Gauss modes. We present a general analytical construction of these states and show the necessary and sufficient condition for them to host embedded dark beams structures. We unveil the intimate connection between discrete rotational symmetry, orbital angular momentum, and the generation of focussing dark beams. The distinguishing features of focussing dark beams are discussed. The potential applications of Discrete-Gauss states in advanced optical trapping and quantum information pro…

PhysicsAngular momentumQuantum PhysicsOperator (physics)GaussianGaussRotational symmetryFOS: Physical sciencesMathematical Physics (math-ph)Atomic and Molecular Physics and OpticsConnection (mathematics)symbols.namesakeClassical mechanicsOptical tweezersQuantum mechanicssymbolsQuantum Physics (quant-ph)Beam (structure)Mathematical PhysicsPhysics - OpticsOptics (physics.optics)
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The broad-line radio galaxy J2114+820

1998

In the frame of the study of a new sample of large angular size radio galaxies selected from the NRAO VLA Sky Survey, we have made radio observations of J2114+820, a low power radio galaxy with an angular size of 6'. Its radio structure basically consists of a prominent core, a jet directed in north-west direction and two extended S-shaped lobes. We have also observed the optical counterpart of J2114+820, a bright elliptical galaxy with a strong unresolved central component. The optical spectrum shows broad emission lines. This fact, together with its low radio power and FR-I type morphology, renders J2114+820 a non-trivial object from the point of view of the current unification schemes of…

NRAO VLA Sky SurveyPhysicsJet (fluid)Active galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysicsSpace and Planetary ScienceAngular diameterElliptical galaxyEmission spectrumAstrophysics::Galaxy AstrophysicsLine (formation)New Astronomy Reviews
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Damping of rotor conical whirl by asymmetric dry friction suspension

2009

Abstract A new technique for the rotor whirl damping in rotating machinery, based on the elastic suspension of the journal boxes and the use of dry friction surfaces normal to the shaft axis between their supports and the frame, is here analysed theoretically for several cases of rotor systems characterized by mass and constraint asymmetry, where gyroscopic effects are to be expected and conical whirl motions may grow up. The critical flexural speeds can be easily cut off by an adhesive state of the supports and the whirl amplitude can be minimized as well throughout the remaining sliding range. Confining the operative angular speed of the rotor in the range of adhesive contact between the …

Materials scienceAcoustics and UltrasonicsRotor (electric)Mechanical EngineeringRotational speedAngular velocityConical surfaceMechanicsDissipationCondensed Matter PhysicsSettore ING-IND/13 - Meccanica Applicata Alle Macchinelaw.inventionRubbingCritical speedClassical mechanicsMechanics of MaterialslawRotating Machinery Gyroscopic Effects Conical Whirl Dry Friction DampersSuspension (vehicle)
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A note on cocharacter sequence of Jordan upper triangular matrix algebra

2016

Let UJn(F) be the Jordan algebra of n × n upper triangular matrices over a field F of characteristic zero. This paper is devoted to the study of polynomial identities satisfied by UJ2(F) and UJ3(F). In particular, the goal is twofold. On one hand, we complete the description of G-graded polynomial identities of UJ2(F), where G is a finite abelian group. On the other hand, we compute the Gelfand–Kirillov dimension of the relatively free algebra of UJ2(F) and we give a bound for the Gelfand–Kirillov dimension of the relatively free algebra of UJ3(F).

Algebra and Number TheoryJordan algebraQuaternion algebraMathematics::Rings and Algebras010102 general mathematicsZero (complex analysis)Triangular matrixgrowth of algebras010103 numerical & computational mathematics01 natural sciencesgraded Jordan algebraCombinatoricsAlgebraFiltered algebraSettore MAT/02 - AlgebraDifferential graded algebraFree algebraAlgebra representationGraded identitie0101 mathematicsMathematics
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Prediction of quantum many-body chaos in protactinium atom

2017

Energy level spectrum of protactinium atom (Pa, Z=91) is simulated with a CI calculation. Levels belonging to the separate manifolds of a given total angular momentum and parity $J^\pi$ exhibit distinct properties of many-body quantum chaos. Moreover, an extremely strong enhancement of small perturbations takes place. As an example, effective three-electron interaction is investigated and found to play a significant role in the system. Chaotic properties of the eigenstates allow one to develop a statistical theory and predict probabilities of different processes in chaotic systems.

PhysicsAtomic Physics (physics.atom-ph)010308 nuclear & particles physicsChaoticFOS: Physical sciencesParity (physics)Configuration interaction01 natural sciencesQuantum chaosPhysics - Atomic PhysicsTotal angular momentum quantum numberQuantum mechanics0103 physical sciencesStatistical theory010306 general physicsQuantumEigenvalues and eigenvectors
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Additivity of effective quadrupole moments and angular momentum alignments in the A~130 nuclei

2007

The additivity principle of the extreme shell model stipulates that an average value of a one-body operator be equal to the sum of the core contribution and effective contributions of valence (particle or hole) nucleons. For quadrupole moment and angular momentum operators, we test this principle for highly and superdeformed rotational bands in the A~130 nuclei. Calculations are done in the self-consistent cranked non-relativistic Hartree-Fock and relativistic Hartree mean-field approaches. Results indicate that the additivity principle is a valid concept that justifies the use of an extreme single-particle model in an unpaired regime typical of high angular momenta.

PhysicsNuclear and High Energy PhysicsAngular momentumValence (chemistry)Nuclear TheorySHELL modelNuclear TheoryFOS: Physical sciencesHartreeNuclear Theory (nucl-th)Additive functionQuantum electrodynamicsQuadrupolePhysics::Atomic and Molecular ClustersAngular momentum operatorNucleon
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Polarization effects in exclusive semi-leptonic Λc and Λb charm and bottom baryon decays

1992

Abstract We discuss polarization effects in semi-leptonic decays of polarized and unpolarized heavy Λ-type baryons into heavy and into light Λ-type baryons. We use the non-leptonic decay of the daughter baryon and the leptonic decay of the Woff-shell into a lepton pair as polarization analyzers to analyze the polarization of the daughter baryon and the Woff-shell. Technically this is done by writing down joint angular decay distributions. We calculate the values of the various asymmetry parameters that characterize the angular dependence of the angular decay distributions where we use the predictions of the heavy quark effective theory (HQET) supplemented by simple ansatze for the q2-depend…

PhysicsNuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectNuclear TheoryHigh Energy Physics::PhenomenologyElementary particlePolarization (waves)AsymmetryBaryonNuclear physicsParticle scatteringHeavy quark effective theoryHigh Energy Physics::ExperimentAngular dependenceNuclear ExperimentLeptonmedia_commonPhysics Letters B
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