Search results for " clusters"

showing 10 items of 1091 documents

All-optical fiber-based devices for ultrafast amplitude jitter magnification

2012

International audience; We propose two fiber-based architectures that enable the all-optical magnification of ultrafast amplitude fluctuations of picosecond or femtosecond pulse trains. An increase of the fluctuations by more than one order of magnitude is experimentally achieved.

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Materials science[ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]business.industryMagnificationPhysics::Optics02 engineering and technology01 natural sciences010309 optics020210 optoelectronics & photonicsAmplitudeOpticsFiber Bragg gratingPicosecond0103 physical sciences0202 electrical engineering electronic engineering information engineeringPhysics::Atomic and Molecular ClustersPhysics::Chemical PhysicsbusinessUltrashort pulseOrder of magnitudeComputingMilieux_MISCELLANEOUSPhotonic-crystal fiberJitter
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Wavelength dependence of multiphoton ionization of xenon

2004

International audience; We have studied the multiphoton ionization of xenon atoms by 160 fs pulses at intensities of 531012 and 1.331013 W/cm2 and present photoelectron kinetic energy and angular distribution spectra measured with a photoelectron imaging spectrometer. A noncollinear optical parametric amplifier allows us to tune the wavelength of the laser pulse over a range between 500 and 700 nm. Resonant and nonresonant processes as well as channel switching effects have been observed in this intensity and wavelength regime. Mainly resonant s5+1d-photon ionization via ns, nd, and nd8 Rydberg states was studied in the region of 505–602 nm. Resonance structures were found related to the tw…

[PHYS.PHYS.PHYS-OPTICS] Physics [physics]/Physics [physics]/Optics [physics.optics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics][ PHYS.PHYS.PHYS-OPTICS ] Physics [physics]/Physics [physics]/Optics [physics.optics]Physics::Atomic and Molecular ClustersPhysics::OpticsPhysics::Atomic Physics
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Echo-assisted impulsive alignment of room-temperature acetone molecules

2021

International audience; We experimentally and theoretically investigate the field-free alignment of the asymmetric-top acetone molecule. Our study shows that the production of postpulse aligned molecules in a dense sample (0.05-0.2 bar) of room-temperature acetone using a single-pulse excitation can be significantly improved by rotational alignment echoes induced in a two-pulse excitation scheme. We report the observation of fractional echoes that can be used to reveal the nonlinearity of the molecular system. In a proof-of-principle experiment, a pre-aligned sample of acetone is also used for third-harmonic generation. The analysis of the experimental data with numerical simulations based …

[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]Materials science[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Echo (computing)[PHYS.PHYS.PHYS-ATM-PH]Physics [physics]/Physics [physics]/Atomic and Molecular Clusters [physics.atm-clus]02 engineering and technology021001 nanoscience & nanotechnology01 natural scienceschemistry.chemical_compoundNuclear magnetic resonancechemistry0103 physical sciencesAcetoneMolecule010306 general physics0210 nano-technology
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Ionization energy of gas phase protein cations and its dependence on charge state_and structure

2013

Ionization energy of gas phase protein cations and its dependence on charge state_and structure. Synchrotron SOLEIL Users Meeting

[SDV.OT]Life Sciences [q-bio]/Other [q-bio.OT][SDV.OT] Life Sciences [q-bio]/Other [q-bio.OT][CHIM.OTHE] Chemical Sciences/Other[ SDU.OTHER ] Sciences of the Universe [physics]/Other[ CHIM.OTHE ] Chemical Sciences/OtherAstrophysics::High Energy Astrophysical PhenomenaPhysics::Atomic and Molecular ClustersPhysics::Accelerator Physics[SDU.OTHER] Sciences of the Universe [physics]/Other[ SDV.OT ] Life Sciences [q-bio]/Other [q-bio.OT]Physics::Chemical Physics[SDU.OTHER]Sciences of the Universe [physics]/Other[CHIM.OTHE]Chemical Sciences/Other
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Rebuilding a Cluster while protecting knowledge within Low-medium-tech supplier SMEs: A Spanish and French comparison

2021

International audience; Most of SMEs are engaged in open innovation practices, but they do not benefit from open innovation or from patenting in the same way as larger firms do. At the same time SMEs, as territorialized suppliers, play a crucial role within evolving regional specialization. In this context the purpose of our study is to examine how low and medium technology supplier SMEs learn and organize themselves at a territorial level to address the challenge of IP protection in an open innovation paradigm. We used a qualitative method with a longitudinal multi-case study involving 27 companies with a historical lance to compare the territorial dynamics of knowledge protection within c…

[SHS.SOCIO]Humanities and Social Sciences/SociologyEnvironmental effects of industries and plantsregional specializationorganizational matrixJEL: R - Urban Rural Regional Real Estate and Transportation EconomicsTJ807-830cooperationlow-medium tech suppliers SMEsintellectual propertyTD194-195regional clusters[SHS.ECO]Humanities and Social Sciences/Economics and FinanceJEL: L - Industrial OrganizationRenewable energy sourcesopen innovationEnvironmental sciencesJEL: O - Economic Development Innovation Technological Change and Growthsocietal path dependency[SHS.GESTION]Humanities and Social Sciences/Business administrationGE1-350Propietat intel·lectual
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NHC-Stabilized Au10 Nanoclusters and Their Conversion to Au25 Nanoclusters

2022

Herein, we describe the synthesis of a toroidal Au10 cluster stabilized by N-heterocyclic carbene and halide ligands via reduction of the corresponding NHC−Au−X complexes (X = Cl, Br, I). The significant effect of the halide ligands on the formation, stability, and further conversions of these clusters is presented. While solutions of the chloride derivatives of Au10 show no change even upon heating, the bromide derivative readily undergoes conversion to form a biicosahedral Au25 cluster at room temperature. For the iodide derivative, the formation of a significant amount of Au25 was observed even upon the reduction of NHC−Au−I. The isolated bromide derivative of the Au25 cluster displays a…

absorptiometal clustersanionitligandsnanohiukkasetliganditgoldanionsabsorptionkulta
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The Gaia-ESO Survey: The origin and evolution of s-process elements

2018

Context. Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations. These trends provide important constraints on stellar and Galactic evolution and they need to be confirmed with large and statistically significant samples of stars spanning wide age and distance intervals. Aims. We aim to trace the abundance patterns and the time evolution of five s-process elements - two belonging to the first peak, Y and Zr, and three belonging to the second peak, Ba, La, and Ce - using the Gaia-ESO IDR5 results for open clusters and disc stars. Methods. From the UVES spectra of cluster member stars, we determined the ave…

astro-ph.GAMetallicityFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: diskAstronomi astrofysik och kosmologiAbundance (ecology)QB4600103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgeneral [Open clusters and associations][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsOpen clusters and associations: generalAstrophysics - Astrophysics of GalaxiesStarsAbundances [Galaxy][SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesAstrophysics::Earth and Planetary AstrophysicsDisk [Galaxy]s-processOpen cluster
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Gaia-ESO Survey: Global properties of clusters Trumpler 14 and 16 in the Carina nebula

2017

Aims: We present the first extensive spectroscopic study of the global population in star clusters Trumpler 16, Trumpler 14, and Collinder 232 in the Carina nebula, using data from the Gaia-ESO Survey, down to solar-mass stars. Methods: In addition to the standard homogeneous survey data reduction, a special processing was applied here because of the bright nebulosity surrounding Carina stars. Results: We find about 400 good candidate members ranging from OB types down to slightly subsolar masses. About 100 heavily reddened early-type Carina members found here were previously unrecognized or poorly classified, including two candidate O stars and several candidate Herbig Ae/Be stars. Their l…

astro-ph.SROpen clusters and associations: individual: Carina nebulaastro-ph.GAExtinction (astronomy)PopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOpen clusters and associations: individual: Trumpler 1401 natural sciencesindividual: Trumpler 16 [Open clusters and associations]Open clusters and associations: individual: Trumpler 16individual: Trumpler 14 [Open clusters and associations]Stars: early-typeearly-type [Stars]pre-main sequence [Stars]QB4600103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)O-type starLine (formation)[PHYS]Physics [physics]PhysicsNebulaeducation.field_of_studyOpen clusters and associations: Individual: Carina nebula; Open clusters and associations: Individual: Trumpler 14; Open clusters and associations: Individual: Trumpler 16; Stars: Early-type; Stars: Pre-main sequence; Astronomy and Astrophysics; Space and Planetary Science010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesStarsStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Stars: pre-main sequenceAstrophysics::Earth and Planetary Astrophysicsindividual: Carina nebula [Open clusters and associations][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon i

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2 Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories for the study of the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion …

astro-ph.SRStellar populationopen clustersand associations: individual: Chamaeleon IIndividual: Chamaeleon I [Open clusters and associations]Open clusters and associations: Individual: Chamaeleon I; Stars: Kinematics and dynamics; Stars: Pre-main sequence; Techniques: Spectroscopicastro-ph.GAstars: kinematics and dynamicsFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequence01 natural sciencesVirial theoremKinematics and dynamics [Stars]Stars: Kinematics and dynamic0103 physical sciencesCluster (physics)Mass segregationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsPre-main sequence [Stars]open clusters and associations: individual: Chamaeleon I010308 nuclear & particles physicsVelocity dispersionAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxies[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]stars: kinematics and dynamics; stars: pre-main sequence; open clustersand associations: individual: Chamaeleon I; techniques: spectroscopicStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsSpectroscopic [Techniques]Equivalent widthtechniques: spectroscopicQB799
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Modelling the effect of nuclear motion on the attosecond time-resolved photoelectron spectra of ethylene

2014

arXiv:1403.5408

attosecond pump probeAttosecondFOS: Physical sciencesElectronmedicine.disease_cause01 natural sciencesSpectral lineSettore FIS/03 - Fisica Della Materianuclear motionTDDFTPhysics - Chemical Physics0103 physical sciencesmedicinePhysics::Atomic and Molecular ClustersMoleculePhysics - Atomic and Molecular ClustersPhysics::Chemical Physics010306 general physicsPhysicsChemical Physics (physics.chem-ph)010304 chemical physicsTRPESTime-dependent density functional theoryCondensed Matter PhysicsAtomic and Molecular Physics and Optics3. Good healthExtreme ultravioletFemtosecondAtomic physicsAtomic and Molecular Clusters (physics.atm-clus)Ultraviolet
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