Search results for " CLUSTER"

showing 10 items of 2162 documents

Distance of matter inside an Einstein-Strauss vacuole

2008

PhysicsSolar masssymbols.namesakeGeodesics in general relativitysymbolsVacuoleAstrophysicsEinsteinGalaxy clusterHubble's law
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First-principles simulations for attosecond photoelectron spectroscopy based on time-dependent density functional theory

2018

We develop a first-principles simulation method for attosecond time-resolved photoelectron spectroscopy. This method enables us to directly simulate the whole experimental processes, including excitation, emission and detection on equal footing. To examine the performance of the method, we use it to compute the reconstruction of attosecond beating by interference of two-photon transitions (RABBITT) experiments of gas-phase Argon. The computed RABBITT photoionization delay is in very good agreement with recent experimental results from [Klünder et al., Phys. Rev. Lett. 106, 143002 (2011)] and [Guénot et al., Phys. Rev. A 85, 053424 (2012)]. This indicates the significance of a fully-consiste…

PhysicsSolid-state physicsAtomic Physics (physics.atom-ph)AttosecondFOS: Physical sciencesObservable02 engineering and technologyPhotoionizationTime-dependent density functional theory021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesSettore FIS/03 - Fisica Della MateriaSpectral linePhysics - Atomic PhysicsElectronic Optical and Magnetic MaterialsX-ray photoelectron spectroscopyRABBIT0103 physical sciencesPhysics::Atomic and Molecular ClustersAtomic physics010306 general physics0210 nano-technologyExcitationThe European Physical Journal B
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Millisecond pulsars in the globular cluster 47 Tucanae

1995

PhysicsSpace and Planetary ScienceMillisecond pulsarGlobular clusterAstronomyAstronomy and AstrophysicsMonthly Notices of the Royal Astronomical Society
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First Glimpse of the N=82 Shell Closure below Z=50 from Masses of Neutron-Rich Cadmium Isotopes and Isomers

2020

We probe the $N=82$ nuclear shell closure by mass measurements of neutron-rich cadmium isotopes with the ISOLTRAP spectrometer at ISOLDE-CERN. The new mass of $^{132}\mathrm{Cd}$ offers the first value of the $N=82$, two-neutron shell gap below $Z=50$ and confirms the phenomenon of mutually enhanced magicity at $^{132}\mathrm{Sn}$. Using the recently implemented phase-imaging ion-cyclotron-resonance method, the ordering of the low-lying isomers in $^{129}\mathrm{Cd}$ and their energies are determined. The new experimental findings are used to test large-scale shell-model, mean-field, and beyond-mean-field calculations, as well as the ab initio valence-space in-medium similarity renormalizat…

PhysicsSpectrometerAb initioShell (structure)Closure (topology)General Physics and AstronomyRenormalization group7. Clean energy01 natural sciencesISOLTRAPIsotopes of cadmium0103 physical sciencesPhysics::Atomic and Molecular ClustersNeutronAtomic physicsNuclear Experiment010306 general physicsPhysical Review Letters
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Electric Field Control of Spin States in Trigonal Two-Electron Quantum Dot Arrays and Mixed-Valence Molecules: II. Vibronic Problem

2018

In this article, the vibronic model for an electric field switchable mixed-valence trimer containing two delocalized electrons or holes is proposed and examined. The role of the vibronic coupling on the electric field effects is analyzed by means of the semiclassical adiabatic approach and, alternatively, with the aid of the numerical analysis of the Schrodinger equation with due allowance for the kinetic energy of the ions (dynamic problem). The adiabatic potential landscapes have been calculated by taking into account the influence of the electric field. As the adiabatic approximation has a limited frame of validity, the study of the electric field effects has also been performed within m…

PhysicsSpin states02 engineering and technologyElectron010402 general chemistry021001 nanoscience & nanotechnology01 natural sciencesMolecular physics0104 chemical sciencesSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsSchrödinger equationAdiabatic theoremsymbols.namesakeDelocalized electronVibronic couplingGeneral EnergyElectric fieldPhysics::Atomic and Molecular ClusterssymbolsPhysical and Theoretical Chemistry0210 nano-technologyAdiabatic processThe Journal of Physical Chemistry C
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Dynamical Casimir-Polder energy between an excited- and a ground-state atom.

2004

We consider the Casimir-Polder interaction between two atoms, one in the ground state and the other in its excited state. The interaction is time-dependent for this system, because of the dynamical self-dressing and the spontaneous decay of the excited atom. We calculate the dynamical Casimir-Polder potential between the two atoms using an effective Hamiltonian approach. The results obtained and their physical meaning are discussed and compared with previous results based on a time-independent approach which uses a non-normalizable dressed state for the excited atom.

PhysicsSpontaneous decayCondensed Matter::Quantum GasesQuantum Physicsquantum fluctuationsFOS: Physical sciencesquantum electrodynamicExcimerAtomic and Molecular Physics and OpticsCasimir effectsymbols.namesakeQuantum mechanicsExcited stateAtomsymbolsPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsAtomic physicsvan der Waals forceHamiltonian (quantum mechanics)Ground stateDynamical Casimir-Polder forceQuantum Physics (quant-ph)
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Nonlocal field correlations and dynamical Casimir-Polder forces between one excited- and two ground-state atoms

2006

The problem of nonlocality in the dynamical three-body Casimir-Polder interaction between an initially excited and two ground-state atoms is considered. It is shown that the nonlocal spatial correlations of the field emitted by the excited atom during the initial part of its spontaneous decay may become manifest in the three-body interaction. The observability of this new phenomenon is discussed.

PhysicsSpontaneous decayQuantum PhysicsField (physics)Dynamical dispersion forceFOS: Physical sciencesThree-body forcesCondensed Matter PhysicsAtomic and Molecular Physics and OpticsCasimir effectQuantum nonlocalityQuantum mechanicsExcited statePhysics::Atomic and Molecular ClustersCausality and nonlocalityPhysics::Atomic PhysicsObservabilityQuantum Physics (quant-ph)Ground state
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The X-ray Luminosity Distributions of the high-metallicity open cluster Blanco 1

2003

We present X-ray Luminosity Distributions (XLDs) of late-type members (dF, dG, dK, dM) of the Blanco 1 cluster, based on ROSAT-HRI data and new astrometric-photometric membership obtained from the GSC-II project. For the first time we present the XLD of dM stars of this cluster. The high metallicity of Blanco 1 allows us to investigate the role of chemical composition on the coronal emission of late-type stars. Comparison between X-ray Luminosity Distributions of Blanco 1 and Pleiades, NGC 2516 and α  Per suggests a possible metallicity effect in dM stars.

PhysicsStarsSpace and Planetary ScienceK-type main-sequence starMetallicityAstronomyAstronomy and AstrophysicsAstrophysicsPleiadesBlue stragglerOpen clusterLuminosity function (astronomy)LuminosityAstronomy & Astrophysics
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The Star Population of Young Open Clusters: A Photometric and Spectroscopic Study

2003

I have determined physical parameters (interstellar reddening, distance, and age) for three young open clusters: h Persei, x Persei, and NGC 1893. I have studied their massive star populations and their formation epochs. I present photometric data for 350 stars in the double open cluster h and x Persei. For both clusters, the distance moduli and reddening are determined to be the same: V0 M p V and E(b y) p . However, the ages for 11.6 0.2 0.42 0.2 the clusters are different. Most stars in h Persei follow the isochrone, although some of the massive stars seem log t p 7.3 younger. By contrast, the stars in x Persei better fit isochrones for (A. Marco & G. Bernabeu 2001, A&A, log t p 7.10–7.1…

PhysicsStarsStar clusterSpace and Planetary ScienceBe starStar formationAstronomyAstronomy and AstrophysicsHerbig Ae/Be starStellar classificationBlue stragglerOpen clusterPublications of the Astronomical Society of the Pacific
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Parameter properties and stellar population of the old open cluster NGC 3960

2004

We present a $BVI$ photometric and astrometric catalogue of the open cluster NGC 3960, down to limiting magnitude $V\sim22$, obtained from observations taken with the Wide Field Imager camera at the MPG/ESO 2.2 m Telescope at La Silla. The photometry of all the stars detected in our field of view has been used to estimate a map of the strong differential reddening affecting this area. Our results indicate that, within the region where the cluster dominates, the $E(V-I)$ values range from 0.21 up to 0.78, with $E(V-I)=0.36$ ($E(B-V)=0.29$) at the nominal cluster centroid position; color excesses $E(V-I)$ up to 1 mag have been measured in the external regions of the field of view where field …

PhysicsStellar populationAstrophysics (astro-ph)CentroidFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsPower lawPhotometry (optics)StarsDistance modulusSpace and Planetary ScienceLimiting magnitudeOpen cluster
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