Search results for "Vector"

showing 10 items of 2660 documents

Solution for an arbitrary number of coupled identical oscillators.

1992

We propose a solution to the problem of solving the Schr\"odinger equation for an arbitrary number of identical one-dimensional harmonically coupled oscillators raised by Fan Hong-yi [Phys. Rev. A 42, 4377 (1990)]. The relationship between the Fock spaces associated with the uncoupled and coupled oscillators is given as well as the coordinate representation of the eigenstates. In view of further applications, the Lie algebraic properties of the model are examined, and the generalization to three spatial dimensions is made.

PhysicsAlgebraic propertiesGeneralizationAtomic and Molecular Physics and OpticsFock spaceSchrödinger equationsymbols.namesakeQuantum mechanicsLie algebrasymbolsRepresentation (mathematics)Eigenvalues and eigenvectorsMathematical physicsThree dimensional modelPhysical review. A, Atomic, molecular, and optical physics
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Analysis of the γγ→DD¯ reaction and the DD¯ bound state

2021

In this work, we investigate the reaction of $\ensuremath{\gamma}\ensuremath{\gamma}\ensuremath{\rightarrow}D\overline{D}$, taking into account the $S$-wave $D\overline{D}$ final state interaction. By fitting to the $D\overline{D}$ invariant mass distributions measured by the Belle and BABAR Collaborations, we obtain a good reproduction of the data by means of a $D\overline{D}$ amplitude that produces a bound $D\overline{D}$ state with isospin $I=0$ close to threshold. The error bands of the fits indicate, however, that more precise data on this reaction are needed to be more assertive about the position and width of such a state.

PhysicsAmplitudePosition (vector)IsospinHigh Energy Physics::PhenomenologyBound stateInvariant massState (functional analysis)Mathematical physicsPhysical Review D
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τ decay into a pseudoscalar and an axial-vector meson

2019

We study theoretically the decay $\tau^- \to \nu_\tau P^- A$, with $P^-$ a $\pi^-$ or $K^-$ and $A$ an axial-vector resonance $b_1(1235)$, $h_1(1170)$, $h_1(1380)$, $a_1(1260)$, $f_1(1285)$ or any of the two poles of the $K_1(1270)$. The process proceeds through a triangle mechanism where a vector meson pair is first produced from the weak current and then one of the vectors produces two pseudoscalars, one of which reinteracts with the other vector to produce the axial resonance. For the initial weak hadronic production we use a recent formalism to account for the hadronization after the initial quark-antiquark pair produced from the weak current, which explicitly filters G-parity states an…

PhysicsAngular momentumMeson010308 nuclear & particles physicsBranching fractionHadronHigh Energy Physics::PhenomenologyG-parity01 natural sciencesPseudoscalarHigh Energy Physics - Phenomenology0103 physical sciencesVector meson010306 general physicsPseudovectorMathematical physics
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Line shape and D(*)D¯(*) probabilities of ψ(3770) from the e+e−→DD¯ reaction

2019

We have performed a calculation of the DD¯, DD¯*, D*D¯, D*D¯* components in the wave function of the ψ(3770). For this we make use of the P03 model to find the coupling of ψ(3770) to these components, that with an elaborate angular momentum algebra can be obtained with only one parameter. Then we use data for the e+e-→DD¯ reaction, from where we determine a form factor needed in the theoretical framework, as well as other parameters needed to evaluate the meson-meson self-energy of the ψ(3770). Once this is done we determine the Z probability to still have a vector core and the probability to have the different meson components. We find Z about 80%–85%, and the individual meson-meson compon…

PhysicsAngular momentumMeson010308 nuclear & particles physicsForm factor (quantum field theory)PropagatorFunction (mathematics)Coupling (probability)01 natural sciences0103 physical sciencesVector meson010306 general physicsWave functionMathematical physicsPhysical Review D
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Orientation of galaxies in structures

2014

The investigation of the orientation of galaxies is a standard test concerning to scenarios of galaxy formation, because different theories of galaxy formation make various predictions regarding to the angular momentum of galaxies. The new method of analysis of the alignment of galaxies in clusters was proposed in the paper Godlowski (2012) and now is improved. We analyzed the distribution of the position angles of the galaxy major axes, as well as the distribution of two angles describing the spatial orientation of galaxy plane, which gives the information about galaxy angular momenta. We discuss the orientation of galaxies in groups and clusters of galaxies. The results show the dependenc…

PhysicsAngular momentumPlane (geometry)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsMethod of analysisAstrophysics - Astrophysics of GalaxiesGalaxyPosition (vector)Astrophysics of Galaxies (astro-ph.GA)Orientation (geometry)Galaxy formation and evolutionStandard testAstrophysics::Galaxy AstrophysicsAstrophysics+
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Preparation of macroscopically distinguishable superpositions of circular or linear oscillatory states of a bidimensionally trapped ion

2000

A simple scheme for the generation of two different classes of bidimensional vibrational Schrodinger cat-like states of an isotropically trapped ion is presented. We show that by appropriately adjusting an easily controllable parameter having a clear physical meaning, the states prepared by our procedure are quantum superpositions of either vibrational axial angular momentum eigenstates or Fock states along two orthogonal directions.

PhysicsAngular momentumsymbols.namesakeSuperposition principleSimple (abstract algebra)Quantum mechanicssymbolsQuantumAtomic and Molecular Physics and OpticsEigenvalues and eigenvectorsSchrödinger's catIonFock spaceJournal of Modern Optics
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Antiproton-proton annihilation at rest in H2 gas into π+ π− π0

1990

Antiproton-proton annihilation at rest into π+ π− π0 has been studied by stopping antiprotons from LEAR in a H2 gas target at normal temperature and pressure. The reaction is observed in coincidence withL X-rays which are emitted in the cascade of\(\bar pp\) atoms. The X-rays populate one of the angular momentumL=1 states of a\(\bar pp\) atom which then annihilates. A spinparity analysis of the π+ π− π0 Dalitz plot gives contributions from the threeP states from which annihilation into three pions is allowed. The most striking features of the Dalitz plot are production of charged and neutral ϱ(770) and off2(1270) mesons. Production of ϱ(770) mesons proceeds via the isoscalar part of the1P1 …

PhysicsAnnihilationPhysics and Astronomy (miscellaneous)IsovectorMesonIsoscalarNuclear TheoryDalitz plotElementary particleNuclear physicsPionAntiprotonHigh Energy Physics::ExperimentNuclear ExperimentEngineering (miscellaneous)Zeitschrift für Physik C Particles and Fields
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A nonlinear eigenvalue problem for the periodic scalar p-Laplacian

2014

We study a parametric nonlinear periodic problem driven by the scalar $p$-Laplacian. We show that if $\hat \lambda_1 >0$ is the first eigenvalue of the periodic scalar $p$-Laplacian and $\lambda> \hat \lambda_1$, then the problem has at least three nontrivial solutions one positive, one negative and the third nodal. Our approach is variational together with suitable truncation, perturbation and comparison techniques.

PhysicsApplied MathematicsScalar (mathematics)AnalysiGeneral MedicineMathematics::Spectral TheoryLambdaSecond deformation theoremParametric equationNonlinear systemp-LaplacianConstant sign and nodal solutionExtremal solutionDivide-and-conquer eigenvalue algorithmParametric equationAnalysisEigenvalues and eigenvectorsParametric statisticsMathematical physics
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Eclipsed X-ray flares in binary stars: geometrical constraints on the flare's location and size

2007

The observation of eclipses during X-rays flares taking place in active cool stars binaries allows us to calculate the position and size of the flares. This information cannot be derived by analyzing the decay of the flares, a frequently used approach in the literature that requires the assumption of a physical model. We make use of the eclipsing light curve to constrain the set of possible solutions, from the geometrical point of view, in two flares of Algol, and one flare in VW Cep. We make use of a technique developed with the system SV Cam (i~90 deg) and generalize it to binary systems with arbitrary inclination. The method simulates all possible geometrical situations that can produce …

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCoronal loopLight curveAstrophysicslaw.inventionStarsSpace and Planetary SciencePosition (vector)lawBinary starPolarAstrophysics::Solar and Stellar AstrophysicsEclipseFlare
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Spectral Analysis of LMC X-2 with XMM-Newton: Unveiling the Emission Process in the Extragalactic Z-source

2008

We present the results of the analysis of an archival observation of LMC X-2 performed with XMM/Newton. The spectra taken by high-precision instruments have never been analyzed before. We find an X-ray position for the source that is inconsistent with the one obtained by ROSAT, but in agreement with the Einstein position and that of the optical counterpart. The correlated spectral and timing behaviour of the source suggests that the source is probably in the normal branch of its X-ray color-color diagram. The spectrum of the source can be fitted with a blackbody with a temperature 1.5 keV plus a disk blackbody at 0.8 keV. Photoelectric absorption from neutral matter has an equivalent hydrog…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsLyman-alpha lineAstrophysicsAstrophysicsSpectral lineBoundary layerSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary SciencePosition (vector)ROSATbinaries accretion accretion disks line: identification stars: neutron [X-rays]Black-body radiationEmission spectrumLarge Magellanic CloudX-rays: binaries accretion accretion disks line: identification stars: neutronAstrophysics::Galaxy Astrophysics
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