Search results for "62"

showing 10 items of 970 documents

Nuclear charge radii and electromagnetic moments of radioactive scandium isotopes and isomers

2011

International audience; Collinear laser spectroscopy experiments with the Sc + transition 3d4s 3 D 2 → 3d4p 3 F 3 at λ = 363.1 nm were performed on the 42−46 Sc isotopic chain using an ion guide isotope separator with a cooler-buncher. Nuclear magnetic dipole and electric quadrupole moments as well as isotope shifts were determined from the hyperfine structure for five ground states and two isomers. Extensive multi-configurational Dirac-Fock calculations were performed in order to evaluate the specific mass-shift, M SMS, and field-shift, F, parameters which allowed evaluation of the charge radii trend of the Sc isotopic sequence. The charge radii obtained show systematics more like the Ti r…

PhysicsNuclear and High Energy Physicscollinear laser spectroscopy010308 nuclear & particles physicschemistry.chemical_element01 natural sciences7. Clean energyEffective nuclear chargeIon21.10.Kychemistrynuclear moments PACS numbers: 21.10.Ft0103 physical sciencesQuadrupolemean-square charge radiusNeutronPhysics::Atomic PhysicsScandium42.62.FiAtomic physics010306 general physicsSpectroscopy32.10.FnMagnetic dipoleHyperfine structureJournal of Physics G: Nuclear and Particle Physics
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Magnetic and quadrupole moments of neutron deficient 58-62Cu isotopes

2011

Abstract This paper reports on the ground state nuclear moments measured in 58–62Cu using collinear laser spectroscopy at the ISOLDE facility. The quadrupole moments for 58–60Cu have been measured for the first time as Q ( Cu 58 ) = − 15 ( 3 ) efm 2 , Q ( Cu 59 ) = − 19.3 ( 19 ) efm 2 , Q ( Cu 60 ) = + 11.6 ( 12 ) efm 2 and with higher precision for 61,62Cu as Q ( Cu 61 ) = − 21.1 ( 10 ) efm 2 , Q ( Cu 62 ) = − 2.2 ( 4 ) efm 2 . The magnetic moments of 58,59Cu are measured with a higher precision as μ ( Cu 58 ) = + 0.570 ( 2 ) μ N and μ ( Cu 59 ) = + 1.8910 ( 9 ) μ N . The experimental nuclear moments are compared to large-scale shell-model calculations with the GXPF1 and GXPF1A effective i…

PhysicsNuclear and High Energy Physicsnuclear-structureIsotopeMagnetic momentNuclear moments010308 nuclear & particles physicsshell-modelNuclear structureN=287. Clean energy01 natural sciencesShell modelCu58Cu59Cu60Cu61Cu620103 physical sciencesQuadrupoleNuclear spinNeutronHyperfine structureAtomic physicsLaser spectroscopy010306 general physicsGround stateSpectroscopyHyperfine structure
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The MuPix high voltage monolithic active pixel sensor for the Mu3e experiment

2015

Mu3e is a novel experiment searching for charged lepton flavor violation in the rare decay μ → eee. In order to reduce background by up to 16 orders of magnitude, decay vertex position, decay time and particle momenta have to be measured precisely. A pixel tracker based on 50 μm thin high voltage monolithic active pixel sensors (HV-MAPS) in a magnetic field will deliver precise vertex and momentum information. Test beam results like an excellent efficiency of >99.5% and a time resolution of better than 16.6 ns obtained with the MuPix HV-MAPS chip developed for the Mu3e pixel tracker are presented.

PhysicsParticle physicsCMOS sensorElectronic detector readout concepts (solid-state)PixelPhysics::Instrumentation and Detectorsbusiness.industryHigh voltageChipElectronic detector readout concepts (solid-state); Particle tracking detectors (solidstate detectors)Magnetic fieldVertex (geometry)OpticsHigh Energy Physics::Experimentddc:610Electric potentialDetectors and Experimental TechniquesParticle tracking detectors (solidstate detectors)ddc:620businessInstrumentationParticle Physics - ExperimentMathematical PhysicsEngineering & allied operationsLepton
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Space-, time- and spin-resolved photoemission

2015

Journal of electron spectroscopy and related phenomena 200, 94 - 118 (2015). doi:10.1016/j.elspec.2015.05.016

PhysicsRadiationbusiness.industrySpace timeDegrees of freedom (physics and chemistry)Spin engineeringPosition and momentum spaceAngle-resolved photoemission spectroscopyElectronCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsComputational physics620MomentumOpticsPhysical and Theoretical Chemistryddc:620businessSpectroscopySpin-½
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On the numerical scheme employed in gyrotron interaction simulations

2012

We report on the influence of the numerical scheme employed in gyrotron interaction simulations. Results obtained with the Crank-Nicolson scheme are compared with those obtained with the Backward Time – Centred Space (BTCS) fully implicit scheme. We present realistic cases where, for discretisation parameters in the range usually used in gyrotron simulations, the results can be very different. Hence, the numerical scheme used can be responsible for obscuring the underlying physics if its convergence is not tested carefully.

PhysicsScheme (programming language)DiscretizationPhysicsQC1-999Space (mathematics)law.inventionlawGyrotronConvergence (routing)Range (statistics)Statistical physicsddc:620computerEngineering & allied operationscomputer.programming_language
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Topological protection of highly entangled non-Gaussian two-photon states

2021

Abstract We study theoretically the evolution of entangled non-Gaussian two-photon states in disordered topological lattices. Specifically, we consider spatially entangled two-photon states, modulated by Laguerre polynomials up to the 3rd order, which feature ring-shaped spatial and spectral correlation patterns. Such states are discrete analogs of photon-subtracted squeezed states, which are ubiquitous in optical quantum information processing or sensing applications. We find that, in general, a higher degree of entanglement coincides with a loss of topological protection against disorder, this is in line with previous results for Gaussian two-photon states. However, we identify a particul…

PhysicsTwo-photon statePhotonGaussianQuantum opticQuantum entanglementParameter spaceTopologyTopological protectionquantum photonicsGaussian stateSettore FIS/03 - Fisica Della Materiasymbols.namesaketopological insulatorsQuantum stateTopological insulatortwo-photon lightsymbolsLaguerre polynomialsddc:621621 Angewandte PhysikQuantum
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A dynamic collimation and alignment system for the Helmholtz linear accelerator

2021

Review of scientific instruments 92(11), 113306 - 113306-9 (2021). doi:10.1063/5.0069824

Physicsbusiness.industryCollimated lightLinear particle accelerator620Transverse planesymbols.namesakeOpticsCryomoduleHelmholtz free energysymbolsContinuous wavePhysics::Accelerator PhysicsThermal emittanceddc:620businessInstrumentationBeam (structure)
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Chandra observation of the Big Dipper X 1624–490

2006

We present the results of a 73 ks long Chandra observation of the dipping source X 1624-490. During the observation a complex dip lasting 4 hours is observed. We analyse the persistent emission detecting, for the first time in the 1st-order spectra of X 1624-490, an absorption line associated to \ion{Ca}{xx}. We confirm the presence of the \ion{Fe}{xxv} K$_\alpha$ and \ion{Fe}{xxvi} K$_\alpha$ absorption lines with a larger accuracy with respect to a previous XMM observation. Assuming that the line widths are due to a bulk motion or a turbulence associated to the coronal activity, we estimate that the lines have been produced in a photoionized absorber between the coronal radius and the out…

Physicsstars : individual : X 1624-490Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysicsAstrophysicsaccretion accretion diskstars : neutronBulk motionSpectral lineIonAccretion discSpace and Planetary ScienceX-rays : starX-rays : binarieindividual : X 1624-490; stars : neutron; X-rays : stars; X-rays : binaries; X-rays : general [accretion accretion disks; stars]X-rays : generalLine (formation)Astronomy & Astrophysics
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Field and numerical study of river confluence flow structures

2010

River hydrodynamics Turbulent open channel flow and transport phenomena

Physics::Fluid DynamicsPhysics::Space PhysicsIngenieurwissenschaften (620)Numerical simulation Large Eddy simulation HydrodynamicsPhysics::Atmospheric and Oceanic PhysicsComputer Science::Information TheoryPhysics::Geophysics
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Reconstruction of events recorded with the surface detector of the Pierre Auger Observatory

2020

Cosmic rays arriving at Earth collide with the upper parts of the atmosphere, thereby inducing extensive air showers. When secondary particles from the cascade arrive at the ground, they are measured by surface detector arrays. We describe the methods applied to the measurements of the surface detector of the Pierre Auger Observatory to reconstruct events with zenith angles less than 60 using the timing and signal information recorded using the water-Cherenkov detector stations. In addition, we assess the accuracy of these methods in reconstructing the arrival directions of the primary cosmic ray particles and the sizes of the induced showers.

Physics::Instrumentation and DetectorsAstronomyprimary [cosmic radiation]01 natural sciences030218 nuclear medicine & medical imagingAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinesurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Data Processing; Large detector systems for particle and astroparticle physics; Large detector-systems performance; Performance of High Energy Physics DetectorsInstrumentationMathematical PhysicsData Processing; Large detector systems for particle and astroparticle physics; Largedetector-systems performance; Performance of High Energy Physics DetectorsLarge detector-systems performanceHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HEInstrumentation et méthodes en physiqueData ProcessingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAugercascadeobservatoryCascadeLargedetector-systems performanceddc:620Astrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenaatmosphere [showers]airAstrophysics::High Energy Astrophysical PhenomenawaterFOS: Physical sciencesCosmic rayAtmosphere03 medical and health sciencesOptics0103 physical sciencesHigh Energy Physics14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Instrumentation and Methods for Astrophysics (astro-ph.IM)ZenithEngineering & allied operationsPierre Auger Observatoryshowers: atmosphere010308 nuclear & particles physicsbusiness.industryhep-exdetector: surfaceLarge detector systems for particle and astroparticle physicsAutres mathématiquescosmic radiation: primaryCherenkov counterExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicHigh Energy Physics::ExperimentPerformance of High Energy Physics Detectorsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSastro-ph.IM
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