Search results for "ample"

showing 10 items of 2398 documents

The X-ray Facility at LAX in Palermo

1996

A description is given of the X-ray facility installed at LAX (Laboratorio per Sperimentazioni con Radiazioni X), jointly operated in Palermo by the DEAF (Department of Energy and Physics Applications) of the University of Palermo and the IFCAT (Institute of Cosmic Physics and Informatics) of the Italian National Research Council. The X-rays are produced by bombarding a target with energized electrons up to 60 keV. Depending on the material of the target, characteristic fluorescence lines as well as continuous bremsstrahlung is emitted. The X-ray beam has an operational energy range of 0,1–25 keV with a flux of 1010–1012 photons/sr · s; the beam, collimated on a length of 10,5 m, has a diam…

PhysicsNuclear physicsStrahlOperational energyResearch councilbusiness.industryElectrical engineeringX-rayCondensed Matter PhysicsSample chamberbusinessSurfaces Coatings and FilmsVakuum in Forschung und Praxis
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Pulsating B and Be Stars in the Magellanic Clouds

2010

Stellar pulsations in main-sequence B-type stars are driven by the κ-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability strips in the B spectral domain at very low metallicities. As the metallicity of the Magellanic Clouds (MC) has been measured to be around Z = 0. 002 for the Small Magellanic Cloud (SMC) and Z = 0. 007 for the Large Magellanic Cloud (LMC), they constitute a very suitable objects to test these predictions. The aim of this work is to investigate the existence of B-type pulsators at low metallicities, searching for short-term periodic variability in a large sample of B and Be stars from the MC with accurately determined f…

PhysicsOpacityAstrophysics::High Energy Astrophysical PhenomenaMetallicitySpectral domainAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsInstabilityLarge sampleStars13. Climate actionAstrophysics::Solar and Stellar AstrophysicsSmall Magellanic CloudLarge Magellanic CloudAstrophysics::Galaxy Astrophysics
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Measurement of the branching fraction of and search for a CP -violating asymmetry in η′→π+π−e+e− at BESIII

2021

The rare decay η′ → π+π−e+e− is studied using a sample of 1.3×109  J/ψ events collected with the BESIII detector at BEPCII in 2009 and 2012. The branching fraction is measured with improved precisi ...

PhysicsParticle physicsBranching fractionmedia_common.quotation_subjectDetectorSample (graphics)Asymmetrymedia_commonPhysical Review D
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Supersymmetry does not imply mass degeneracy

2004

Abstract It is commonly believed that unbroken supersymmetry (SUSY) implies that all members of a supermultiplet have the same mass. We demonstrate that this is not true, by exhibiting a simple counterexample. We employ the formalism of homeotic fermions, in a simple model where CPT conjugate fermions have different masses. This model can be supersymmetrized to a hypermultiplet of fields which form a representation of the conventional N=2 SUSY algebra. Nevertheless, CPT conjugate states in this hypermultiplet have different masses. These surprising results do not violate either the CPT theorem or the Haag–Lopuszanski–Sohnius theorem.

PhysicsParticle physicsNuclear and High Energy PhysicsCPT symmetryHypermultipletHigh Energy Physics::PhenomenologyFísicaSupersymmetryFermionTheoretical physicsFormalism (philosophy of mathematics)High Energy Physics::TheorySupermultipletHigh Energy Physics::ExperimentCounterexampleSupersymmetry algebraPhysics Letters B
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Search for the DecayB+→K+νν¯

2005

We search for the rare flavor-changing neutral-current decay ${B}^{+}\ensuremath{\rightarrow}{K}^{+}\ensuremath{\nu}\overline{\ensuremath{\nu}}$ in a data sample of $82\text{ }\text{ }{\mathrm{fb}}^{\ensuremath{-}1}$ collected with the BABAR detector at the PEP-II $B$-factory. Signal events are selected by examining the properties of the system recoiling against either a reconstructed hadronic or semileptonic charged-$B$ decay. Using these two independent samples we obtain a combined limit of $\mathcal{B}({B}^{+}\ensuremath{\rightarrow}{K}^{+}\ensuremath{\nu}\overline{\ensuremath{\nu}})l5.2\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}$ at the 90% confidence level. In addition, by…

PhysicsParticle physicsPion010308 nuclear & particles physicsElectron–positron annihilation0103 physical sciencesHadronIndependent samplesGeneral Physics and Astronomy010306 general physics01 natural sciencesReconstruction methodPhysical Review Letters
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Solution of the Lindblad equation in Kraus representation

2006

The so-called Lindblad equation, a typical master equation describing the dissipative quantum dynamics, is shown to be solvable for finite-level systems in a compact form without resort to writing it down as a set of equations among matrix elements. The solution is then naturally given in an operator form, known as the Kraus representation. Following a few simple examples, the general applicability of the method is clarified.

PhysicsQuantum PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciLindblad equationFOS: Physical sciencesAtomic and Molecular Physics and OpticsSettore FIS/03 - Fisica Della MateriaThe so-called Lindblad equation a typical master equation describing the dissipative quantum dynamics is shown to be solvable for finite-level systems in a compact form without resort to writing it down as a set of equations among matrix elements. The solution is then naturally given in an operator form known as the Kraus representation. Following a few simple examples the general applicability of the method is clarified.Open quantum systemQuantum processMaster equationDissipative systemQuantum operationMethod of quantum characteristicsQuantum Physics (quant-ph)Quantum statistical mechanicsMathematical physics
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Does the galaxy correlation length increase with the sample depth?

2001

We have analyzed the behavior of the correlation length, $r_0$, as a function of the sample depth by extracting from the CfA2 redshift survey volume--limited samples out to increasing distances. For a fractal distribution, the value of $r_0$ would increase with the volume occupied by the sample. We find no linear increase for the CfA2 samples of the sort that would be expected if the Universe preserved its small scale fractal character out to the distances considered (60--100$\hmpc$). The results instead show a roughly constant value for $r_0$ as a function of the size of the sample, with small fluctuations due to local inhomogeneities and luminosity segregation. Thus the fractal picture ca…

PhysicsSample (material)Astrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsFunction (mathematics)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRedshift surveyGalaxyLuminosityFractalDistribution (mathematics)Space and Planetary ScienceConstant (mathematics)
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The Computer Code for Calculations of the Positron Distribution in a Layered Stack Systems

2014

In this paper we present experimental and theoretical studies of the implantation pro le of positrons emitted fromNa radionuclide into layered sample. The measured pro le for the nonsymmetrical, around the positron emitter, stack of aluminium and silver foils was measured using the depth scanning of implantation pro le technique. For the description of the obtained results two theoretical approaches were applied. The rst one was the Monte Carlo simulation using the GEANT4 tool kit. The generated pro le does not reproduce accurately the experimental pro le. We proposed the multiple scattering model based on the fact that a positron due to backscattering can travel as an energetic particle se…

PhysicsSource codeScatteringmedia_common.quotation_subjectMonte Carlo methodGeneral Physics and AstronomySample (graphics)Computational physicsPositronStack (abstract data type)Physics::Accelerator PhysicsParticleAbsorption (electromagnetic radiation)media_commonActa Physica Polonica A
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Absolute kinematics of radio source components in the complete S5 polar cap sample

2004

We observed the thirteen extragalactic radio sources of the complete S5 polar cap sample at 15.4 GHz with the Very Long Baseline Array, on 27 July 1999 (1999.57) and 15 June 2000 (2000.46). We present the maps from those two epochs, along with maps obtained from observations of the 2 cm VLBA survey for some of the sources of the sample, making a total of 40 maps. We discuss the apparent morphological changes displayed by the radio sources between the observing epochs. Our VLBA observations correspond to the first two epochs at 15.4 GHz of a program to study the absolute kinematics of the radio source components of the members of the sample, by means of phase delay astrometry at 8.4 GHz, 15.…

PhysicsSpectral indexInterferometricAstronomy and AstrophysicsAstrometryKinematicsAstrometryAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGalaxies:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Sample (graphics)Radio continuumSpace and Planetary ScienceBL Lacertae objectsAstrometry ; Interferometric ; Galaxies ; Quasars ; BL Lacertae objects ; Radio continuumUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaPolar capQuasars:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Very Long Baseline ArrayGroup delay and phase delayAstronomy & Astrophysics
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Open inquiry-based learning experiences: a case study in the context of energy exchange by thermal radiation

2013

An open inquiry (OI)-based teaching/learning experience, regarding a scientific investigation of the process of energy exchange by thermal radiation, is presented. A sample of upper secondary school physics teachers carried out this experience at the University of Palermo, Italy, in the framework of ESTABLISH, a FP7 European Project aimed at promoting and developing inquiry-based science education. The teachers had the opportunity to personally experience an OI-based learning activity, with the aim of exploring the pedagogical potentialities of this teaching approach to promote both the understanding of difficult concepts and a deeper view of scientific practices. The teachers were firstly …

PhysicsThermal RadiationProcess (engineering)Settore FIS/08 - Didattica E Storia Della Fisica4. EducationPerspective (graphical)General Physics and AstronomySample (statistics)Context (language use)Science educationInquiry Based Science EducationPhysics EducationTeacher EducationStructured interviewMathematics educationInquiry-based learningEnergy exchangeEuropean Journal of Physics
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