Search results for "Variable"

showing 10 items of 1674 documents

Hβ photometry for UVBY standard stars

1988

From 1984 to 1986 the authors made several observational campaigns at Calar Alto and La Palma Observatories using the uvby and β photometric systems to monitor a selected sample of late-type variable stars. In this paper they present the β values for 38 uvby standard stars to contribute to the uvby-β calibration works on late-type stars. In the final discussion, the β computed values are plotted against the Stroemgren b-y, m_(1), and c_(1) indices.

PhysicsAstrofísicaAstronomíaStarsPhotometry (astronomy)Space and Planetary ScienceAstronomy and AstrophysicsBeta (velocity)AstrophysicsVariable star
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Long-term variability of the Be/X-ray binary A 0535+26 -- I. Optical and UV spectroscopy

1998

The results of a 7-yr optical and UV spectroscopic study of the high-mass X-ray binary A 0535+26 are presented. It was found that throughout the period of the observations the line profile of Hα showed considerable variability. A correlation between the equivalent width of Hα and both V-band magnitude and (B−V) colour excess was observed, albeit with considerable scatter present in the data set. A giant X-ray flare in early 1994 was accompanied by a fading in optical and infrared photometric bands, and a reduction in the equivalent width of Hα. When the star was observed in 1994 September, it was found to have developed a double-peaked Hα profile, and further observations saw the V/R peak r…

PhysicsBe starX-ray binaryAstronomyAstronomy and AstrophysicsAstrophysicsAstronomical spectroscopylaw.inventionSpace and Planetary SciencelawAstrophysics::Solar and Stellar AstrophysicsH-alphaVariable starEquivalent widthAstrophysics::Galaxy AstrophysicsFlareLine (formation)Monthly Notices of the Royal Astronomical Society
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An optimized Bell test in a dynamical system

2010

The best realization of a Bell test depends on parameters linked to experimental settings. We report, for a class of two-qubit states, some optimized parameters that are useful to perform an optimized Bell test in a dynamical context. The time evolution of these optimized parameters, that present finite jumps, is investigated for two qubits in separated cavities.

PhysicsBell stateSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciGeneral Physics and AstronomyContext (language use)Quantum PhysicsQuantum entanglementBell testClassical mechanicsLocal hidden variable theoryOpen quantum systemNonlocalityBell test experimentsStatistical physicsGHZ experimentRealization (systems)Quantum teleportationPhysics Letters A
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Central role of the observable electric potential in transport equations.

2001

Nonequilibrium systems are usually studied in the framework of transport equations that involve the true electric potential (TEP), a nonobservable variable. Nevertheless another electric potential, the observable electric potential (OEP), may be defined to construct a useful set of transport equations. In this paper several basic characteristics of the OEP are deduced and emphasized: (i) the OEP distribution depends on thermodynamic state of the solution, (ii) the observable equations have a reference value for all other transport equations, (iii) the bridge that connects the OEP with a certain TEP is usually defined by the ion activity coefficient, (iv) the electric charge density is a non…

PhysicsClassical mechanicsDistribution (mathematics)Thermodynamic statePhysics::Atomic and Molecular ClustersNon-equilibrium thermodynamicsCharge densityObservableStatistical physicsElectric potentialIonVariable (mathematics)Physical review. E, Statistical, nonlinear, and soft matter physics
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Canonical Adiabatic Theory

2001

In the present chapter we are concerned with systems, the change of which—with the exception of a single degree of freedom—should proceed slowly. (Compare the pertinent remarks about \(\varepsilon\) as slow parameter in Chap. 7) Accordingly, the Hamiltonian reads: $$\displaystyle{ H = H_{0}{\bigl (J,\varepsilon p_{i},\varepsilon q_{i};\varepsilon t\bigr )} +\varepsilon H_{1}{\bigl (J,\theta,\varepsilon p_{i},\varepsilon q_{i};\varepsilon t\bigr )}\;. }$$ (12.1) Here, \((J,\theta )\) designates the “fast” action-angle variables for the unperturbed, solved problem \(H_{0}(\varepsilon = 0),\) and the (p i , q i ) represent the remaining “slow” canonical variables, which do not necessarily have…

PhysicsCombinatoricssymbols.namesakeCanonical variableCanonical coordinatessymbolsAction-angle coordinatesAdiabatic processHamiltonian (quantum mechanics)
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A three-dimensional smoothed particle hydrodynamics simulation of the active phase of SS Cyg-type discs and its implications for the mass transfer bu…

1993

We perform a smoothed particle hydrodynamics (SPH) three-dimensional simulation of the outburst phase of the accretion disc of a typical SS Cyg-like dwarf nova in the framework of the mass transfer burst model (MTBM), where we assume that the active phase is triggered by a sudden increase in the accretion rate due to some instability in the secondary's atmosphere. The evolution of the accretion disc is followed for a single orbital period, starting from the initial quiescent disc configuration obtained by us in a previous paper. This is a suitable integration time for determining the geometrical and physical properties of the disc in the impulsive phase and is comparable with observed outbu…

PhysicsComputer simulationAstrophysics::High Energy Astrophysical PhenomenaCataclysmic variable starAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsOrbital periodInstabilityAccretion (astrophysics)Smoothed-particle hydrodynamicsSpace and Planetary ScienceMass transferAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsDwarf novaAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Free-fall expansion of finite-temperature Bose-Einstein condensed gas in the non Thomas-Fermi regime

2008

We report on our study of the free-fall expansion of a finite-temperature Bose-Einstein condensed cloud of 87Rb. The experiments are performed with a variable total number of atoms while keeping constant the number of atoms in the condensate. The results provide evidence that the BEC dynamics depends on the interaction with thermal fraction. In particular, they provide experimental evidence that thermal cloud compresses the condensate.

PhysicsCondensed Matter::Quantum GasesCondensed matter physicsCondensed Matter::OtherFOS: Physical sciencesFraction (chemistry)Condensed Matter PhysicsAtomic and Molecular Physics and Opticslaw.inventionCondensed Matter - Other Condensed MatterlawThermalConstant (mathematics)Bose–Einstein condensateOther Condensed Matter (cond-mat.other)Fermi Gamma-ray Space TelescopeVariable (mathematics)
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Low-energy excitations from interacting tunneling units in the mean-field approximation

1991

Abstract The low-energy excitation spectrum of dilute concentrations of interacting tunneling quadrupoles randomly distributed in a non-polar medium was studied in the mean-field approximation. In particular the case of six-orientational tunneling quadrupoles (TQs) with a r−3 (elastic) interaction was considered. Because of the random position of the TQs, the internal field in a random variable and for relatively low concentrations has a Lorenzian probability distribution. The low-energy density of states is a constant and the low-energy excitations arise from the large internal fields, i.e. strongly interacting tunneling quadrupoles. The low-energy excitations were compared with those obta…

PhysicsCondensed matter physicsField (physics)Condensed Matter PhysicsElectronic Optical and Magnetic MaterialsMean field theoryMaterials ChemistryCeramics and CompositesDensity of statesVirial expansionProbability distributionAtomic physicsRandom variableQuantum tunnellingExcitationJournal of Non-Crystalline Solids
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Clustering of Sloan Digital Sky Survey III Photometric Luminous Galaxies: The Measurement, Systematics and Cosmological Implications

2012

The Sloan Digital Sky Survey (SDSS) surveyed 14,555 square degrees, and delivered over a trillion pixels of imaging data. We present a study of galaxy clustering using 900,000 luminous galaxies with photometric redshifts, spanning between $z=0.45$ and $z=0.65$, constructed from the SDSS using methods described in Ross et al. (2011). This data-set spans 11,000 square degrees and probes a volume of $3h^{-3} \rm{Gpc}^3$, making it the largest volume ever used for galaxy clustering measurements. We present a novel treatment of the observational systematics and its applications to the clustering signals from the data set. In this paper, we measure the angular clustering using an optimal quadrati…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cepheid variablemedia_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesFísicaAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLambdaRedshiftGalaxySettore FIS/05 - Astronomia e AstrofisicaSpace and Planetary ScienceSkyBaryon acoustic oscillationsNeutrinoAstrophysics::Galaxy Astrophysicsmedia_commonAstrophysics - Cosmology and Nongalactic Astrophysics
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Nondegeneracy in the Perturbation Theory of Integrable Dynamical Systems

1990

The most general nondegeneracy condition for the existence of invariant tori in nearly integrable and analytic Hamiltonian systems is formulated.

PhysicsDynamical systems theoryIntegrable systemMathematics::Complex VariablesQuantum mechanicsTorusInvariant (physics)Mathematics::Symplectic GeometryHamiltonian systemMathematical physics
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