Search results for "Application"

showing 10 items of 5559 documents

Neutron cross section measurements at n_TOF for ADS related estudies

2005

A neutron Time-of-Flight facility (n_TOF) is available at CERN since 2001. The innovative features of the neutron beam, in particular the high instantaneous flux, the wide energy range, the high resolution and the low background, make this facility unique for measurements of neutron induced reactions relevant to the field of Emerging Nuclear Technologies, as well as to Nuclear Astrophysics and Fundamental Nuclear Physics. The scientific motivations that have led to the construction of this new facility are here presented. The main characteristics of the n_TOF neutron beam are described, together with the features of the experimental apparata used for cross-section measurements. The main res…

HistoryAstrofísica nuclearNeutron cross sectionsNuclear transmutationNuclear engineeringNuclear TheoryNuclear physicsNeutrons -- SeccionsEducationNuclear physicsRadiació ionitzant -- Mesures de seguretatRadioactive wastesNeutron cross sectionNuclear astrophysicsNeutronNuclear ExperimentPhysicsLarge Hadron Collider:Física [Àrees temàtiques de la UPC]Time-of-flight mass spectrometryRadioactive wasteNeutron radiationWaste disposalResidus radioactiusComputer Science ApplicationsShielding (Radiation)Physics::Accelerator PhysicsNuclear astrophysicsFísica nuclearNucleon
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Highlights from the ARGO-YBJ Experiment

2012

""The ARGO-YBJ experiment at YangBaJing in Tibet (4300m a.s.l.) has been taking data with its full layout since October 2007. Here we present a few significant results obtained in gamma-ray astronomy and cosmic-ray physics. Emphasis is placed on the analysis of gamma-ray emission from point-like sources (Crab Nebula, MRK 421), on the preliminary limit on the antiproton\\\/proton flux ratio, on the large-scale cosmic-ray anisotropy and on the proton-air cross-section. The performance of the detector is also discussed, and the perspectives of the experiment are outlined.""

HistoryAstronomyFluxAstrophysicsProton flux01 natural sciencesArgo-YbjGamma-ray emissionSettore FIS/05 - Astronomia E AstrofisicaCosmic-ray physicsResistive Plate ChambersInstrumentation010303 astronomy & astrophysicsArgoPhysicsRange (particle radiation)DetectorSettore FIS/01 - Fisica SperimentaleCrab nebulaAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayCrab nebula Extensive air showers Flux ratio Gamma-ray astronomy Gamma-ray emission Ground based Resistive plate chambers; Astronomy Cosmic rays Cosmology Experiments; Gamma raysFlux ratioCosmologyComputer Science ApplicationsResistive plate chambersNuclear and High Energy PhysicsX- and γ-ray instrumentGround-based gamma-ray astronomyAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsCosmic RayEducationResistive Plate Chambers Extensive air showers Ground-based g ray astronomy Cosmic-ray physicsGround-based γ-ray astronomy0103 physical sciencesExtensive air showersCosmic raysExtensive air showers X- and γ-ray instruments Pulsars. Quasars active or peculiar galaxies objects and systemsAstrophysics::Galaxy AstrophysicsGamma-ray astronomy010308 nuclear & particles physicsGamma raysAstronomyResistive Plate ChamberGround basedCrab NebulaAntiprotonResistive Plate Chambers; Extensive air showers; Ground-based γ-ray astronomy; Cosmic-ray physicsSatelliteGamma-ray burstExperimentsJournal of Physics: Conference Series
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Temperature dependence of sodium and ionized calcium resonance lines perturbed by helium

2014

International audience; Traces of heavy metals in cool DZ white dwarf stars may be attributed to the accretion of circumstellar dust thought to originate from tidal disruption of rocky parent bodies. Spectra of such stars therefore provide a unique opportunity to study the composition of extrasolar planetary systems. The determination of metal abundances from stellar spectra depends on stellar atmospheric parameters and an accurate prior knowledge of the collision broadening of the line profiles by the most common constituents of the stellar atmosphere. For this purpose, we present theoretical absorption spectra of Na and Ca+ broadened by He for the conditions prevailing in cool white dwarf…

HistoryAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsHelium01 natural sciencesAstronomical spectroscopySpectral lineEducation0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics][PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]ChemistryStellar atmosphereWhite dwarfAstronomyPlanetary system[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Accretion (astrophysics)Computer Science ApplicationsStars13. Climate actionCircumstellar dustAtomic and molecular collisions[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Astrophysics::Earth and Planetary AstrophysicsMolecular physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Journal of Physics: Conference Series
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Conservative upper limits on WIMP annihilation cross section from Fermi-LAT $γ$-rays

2011

The spectrum of an isotropic extragalactic {\gamma}-ray background (EGB) has been measured by the Fermi-LAT telescope at high latitudes. Two new models for the EGB are derived from the subraction of unresolved point sources and extragalactic diffuse processes, which could explain from 30% to 70% of the Fermi-LAT EGB. Within the hypothesis that the two residual EGBs are entirely due to the annihilation of dark matter (DM) particles in the Galactic halo, we obtain stringent upper limits on their annihilation cross section. Severe bounds on a possible Sommerfeld enhancement of the annihilation cross section are set as well. Finally, we consider models for DM annihilation depending on the inver…

HistoryAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesEducationlaw.inventionGalactic haloTelescopeCross section (physics)WIMPlaw0103 physical sciences010306 general physicsAstrophysics::Galaxy AstrophysicsPhysicsastro-ph.HEAnnihilation010308 nuclear & particles physicsIsotropyhep-phComputer Science ApplicationsHigh Energy Physics - PhenomenologyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsFermi Gamma-ray Space Telescope
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The next generation of laser spectroscopy experiments using light muonic atoms

2018

Precision spectroscopy of light muonic atoms provides unique information about the atomic and nuclear structure of these systems and thus represents a way to access fundamental interactions, properties and constants. One application comprises the determination of absolute nuclear charge radii with unprecedented accuracy from measurements of the 2S - 2P Lamb shift. Here, we review recent results of nuclear charge radii extracted from muonic hydrogen and helium spectroscopy and present experiment proposals to access light muonic atoms with Z ≥ 3. In addition, our approaches towards a precise measurement of the Zemach radii in muonic hydrogen (μp) and helium (μ 3He+) are discussed. These resul…

HistoryAtomic Physics (physics.atom-ph)measurement methodschemistry.chemical_elementFOS: Physical sciences01 natural sciencesEffective nuclear chargeEducationLamb shiftPhysics - Atomic Physicshydrogen: muonic atom0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysics::Atomic Physics010306 general physicsSpectroscopyHeliumExotic atomPhysics[PHYS]Physics [physics]010308 nuclear & particles physicsPrecision spectroscopyhelium: muonic atomnucleusNuclear structureFundamental interaction[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Computer Science ApplicationsLamb shiftlaserchemistrycharge radiusquantum electrodynamics: bound statespectrometerAtomic physicsexperimental results
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Workshop on Sources of Polarized Leptons and High Brightness Electron Beams

2011

This volume contains the proceedings of the International Workshop on Sources of Polarized Leptons and High Brightness Electron Beams (PESP2010). The workshop was hosted by the University of Bonn from 21–24 September 2010. PESP2010 has been conducted as satellite workshop preceding the International SPIN Physics Symposium (SPIN2010). In view of the expanding and challenging field of the production of high brightness lepton beams, the selection of workshop topics was extended to cover the demands of modern accelerator developments and applications. As novel light sources such as FELs and ERLs place new requirements on the properties of unpolarized beams in terms of brightness and intensity, …

HistoryBrightnessEngineeringbusiness.industrymedia_common.quotation_subjectAdvisory committeeEngineering physicsComputer Science ApplicationsEducationPresentationTelecommunicationsbusinessmedia_commonLeptonJournal of Physics: Conference Series
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Interpretation of EXAFS in ReO3using molecular dynamics simulations

2009

Temperature dependent Re L3-edge EXAFS signals from perovskite-type cubic ReO3 have been successfully interpreted using a combination of classical NVT molecular dynamics (MD) and ab initio multiple-scattering approach. The force field model, required for MD simulations, has been determined by fitting the Re-O and O-O pairwise interatomic potentials to a set of experimental data (lattice parameter, elastic constants and bulk modulus) and phonon frequencies, theoretically calculated from the first principles at high symmetry points of the Brillouin zone. The MD simulations reproduce well the anisotropy of thermal vibration for oxygen atoms and confirm a deviation of the mean Re-O-Re angle fro…

HistoryBulk modulusCondensed matter physicsPhononChemistryAb initioMolecular physicsForce field (chemistry)Computer Science ApplicationsEducationBrillouin zoneCondensed Matter::Materials ScienceMolecular dynamicsLattice constantAnisotropyJournal of Physics: Conference Series
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Omnibus experiment: CPT and CP violation with sterile neutrinos

2017

The verification of the sterile neutrino hypothesis and, if confirmed, the determination of the relevant oscillation parameters is one of the goals of the neutrino physics in near future. We propose to search for the sterile neutrinos with a high statistics measurement utilizing the radioactive sources and oscillometric approach with large liquid scintillator detector like LENA, JUNO, or RENO-50. Our calculations indicate that such an experiment is realistic and could be performed in parallel to the main research plan for JUNO, LENA, or RENO-50. Assuming as the starting point the values of the oscillation parameters indicated by the current global fit (in 3 + 1 scenario) and requiring at le…

HistoryCP violationPhysics::Instrumentation and Detectorssterile neutrinosneutrino oscillometryHigh Energy Physics::PhenomenologyneutriinotHigh Energy Physics::ExperimentCPT violationComputer Science ApplicationsEducationJournal of Physics: Conference Series
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Application of micro Raman spectroscopy to industrial FC membranes

2007

Raman spectra of as-received and protonated membranes (Nafion® NRE-212, Fumapem® F-14100 and Fumasep® FAA) were measured with He-Cd and Ar laser. For the first time the Raman and IR spectra are reported of Fumasep membranes. Most of peaks in vibration spectra active in Raman and IR of membranes are interpreted with C-F, C-S, C-O-C, SO3, C-C bonds. The vibration region connected with protons and H-O bond in both types of membranes is found in Raman and IR spectra.

HistoryChemistryAnalytical chemistryInfrared spectroscopyProtonationVibration spectraLaserComputer Science ApplicationsEducationMicro raman spectroscopylaw.inventionsymbols.namesakeMembranelawsymbolsRaman spectroscopyJournal of Physics: Conference Series
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High-precision mass measurements for fundamental applications using highly-charged ions with SMILETRAP

2007

The Penning trap mass spectrometer SMILETRAP takes advantage of highly-charged ions for high-accuracy mass measurements. In this paper recent mass measurements on Li and Ca ions are presented and their impact on fundamental applications discussed, especially the need for accurate mass values of hydrogen-like and lithium-like ions in the evaluation of the electron g-factor measurements in highly-charged ions is emphasized. Such experiments aim to test bound state quantum electrodynamics. Here the ionic mass is a key ingredient, which can be the limiting factor for the final precision.

HistoryChemistryBound stateIonic bondingElectronIon trapAtomic physicsPenning trapMass spectrometryComputer Science ApplicationsEducationIonJournal of Physics: Conference Series
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