Search results for "530"

showing 10 items of 1476 documents

On-Surface Reactions

2015

On-surface synthesis constitutes a rapidly growing field of research due to its promising application for creating stable molecular structures on surfaces. While self-assembled structures rely on reversible interactions, on-surface synthesis provides the potential for creating long-term stable structures with well-controlled properties, for example superior electron transport for future molecular electronic devices. On-surface synthesis holds the promise for preparing insoluble compounds that cannot be produced in solution. Another highly exciting aspect of on-surface synthesis is the chance to discover new reaction pathways due to the two-dimensional confinement of the reaction educts. In …

molecular electronicsChemistryMolecular electronicsNanotechnologySurface reaction530Atomic and Molecular Physics and Opticstwo-dimensional confinementmolecular structure formationmicroscopyElectronicsscanning probePhysical and Theoretical Chemistryultrahigh vacuumHigh potentialChemPhysChem
researchProduct

Search for Electron Antineutrino Appearance in a Long-baseline Muon Antineutrino Beam

2020

Electron antineutrino appearance is measured by the T2K experiment in an accelerator-produced antineutrino beam, using additional neutrino beam operation to constrain parameters of the Pontecorvo-Maki-Nakagawa-Sakata (PMNS) mixing matrix. T2K observes 15 candidate electron antineutrino events with a background expectation of 9.3 events. Including information from the kinematic distribution of observed events, the hypothesis of no electron antineutrino appearance is disfavored with a significance of 2.40 σ and no discrepancy between data and PMNS predictions is found. A complementary analysis that introduces an additional free parameter which allows non-PMNS values of electron neutrino and a…

muon antineutrino beamGeneral Physics and Astronomyantineutrino/mu: secondary beamKAMIOKANDEantineutrino/e: particle identification01 natural sciences09 EngineeringHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)secondary beam [neutrino/mu][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino/e: particle identificationQCPhysics02 Physical SciencesPhysicsJ-PARC LabT2K experimentelectron antineutrinoT2K CollaborationkinematicsPhysical SciencesParticle Physics - ExperimentT2K experiment in an accelerator-producedGeneral Physics530 PhysicsPhysics MultidisciplinaryFOS: Physical sciencesparticle identification [antineutrino/e]Neutrino beamsecondary beam [antineutrino/mu]530Physics::GeophysicsNuclear physics0103 physical sciencesmixingddc:530010306 general physics01 Mathematical SciencesMuonScience & Technologyparticle identification [neutrino/e]hep-exbackgroundHigh Energy Physics - Experiment; High Energy Physics - Experimentneutrino/mu: secondary beamantineutrino: oscillationoscillation [antineutrino]Elementary Particles and FieldsHigh Energy Physics::ExperimentPMNSElectron neutrinoBeam (structure)Free parameterexperimental results
researchProduct

Design and implementation of the AMIGA embedded system for data acquisition

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and admin-istrative staff in Malargtie. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energla Atomica, Agencia Nacional de Promocion Cientffica y Tec-nologica (ANPCyT) , Consejo Nacional de Investigaciones Cientfficas y Tecnicas (CONICET) , Gobierno de la Provincia de Mendoza, Municipalidad de Malargtie, NDM Holdings and Valle Las Leilas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho…

muon: showersDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Physics::Instrumentation and Detectorsdata acquisitionAstronomycosmic radiation: electromagnetic componentengineeringprimary [cosmic radiation]Particle detectors01 natural sciencesenergy: thresholdData acquisition concepthardwareInstrumentationMathematical Physicsshowers [muon]media_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEControl and monitor systems onlinePhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsthreshold [energy]16. Peace & justiceAugerelectromagnetic component [cosmic radiation]observatoryDetector control systems (detector andexperiment monitoring and slow-control systemslanguageupgradeAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)atmosphere [showers]Land accessarchitectureEuropean communityairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalgorithmsPolitical science0103 physical sciencesmedia_common.cataloged_instanceddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Control and monitor systems online; Data acquisition concepts; Detector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases); Particle detectorsEuropean union010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Ciencias Exactasscintillation countershowers: atmosphere010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsData acquisition conceptsFísicastabilitylanguage.human_languagecosmic radiation: primarymonitoringResearch councilExperimental High Energy PhysicsHigh Energy Physics::ExperimentControl and monitor systems on-linePortuguese[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HumanitiesRAIOS CÓSMICOSastro-ph.IM
researchProduct

Calibration of the underground muon detector of the Pierre Auger Observatory

2021

To obtain direct measurements of the muon content of extensive air showers with energy above $10^{16.5}$ eV, the Pierre Auger Observatory is currently being equipped with an underground muon detector (UMD), consisting of 219 10 $\mathrm{m^2}$-modules, each segmented into 64 scintillators coupled to silicon photomultipliers (SiPMs). Direct access to the shower muon content allows for the study of both of the composition of primary cosmic rays and of high-energy hadronic interactions in the forward direction. As the muon density can vary between tens of muons per m$^2$ close to the intersection of the shower axis with the ground to much less than one per m$^2$ when far away, the necessary bro…

muon: showersdata acquisitionPhysics::Instrumentation and DetectorsAstronomyDetector alignment and calibration methods (lasers sources particle-beams)primary [cosmic radiation]Particle detectors7. Clean energy01 natural sciencesEtc)030218 nuclear medicine & medical imaging0302 clinical medicinecalibration [detector]ObservatoryAPDsdetector: calibrationatmosphere [muon]InstrumentationPhoton detectors for UVshowers [muon]Mathematical PhysicsPhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDsSi-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Particle-beams)Physicsenergy: highdetector [muon]EBCCDsPhysicselectronicsSettore FIS/01 - Fisica SperimentalePhoton detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc)Astrophysics::Instrumentation and Methods for AstrophysicsSourcesSi-PMTsdetector: alignmentAugermuon: atmosphereobservatorydensity [muon]G-APDshigh [energy]Particle detectorAstrophysics - Instrumentation and Methods for Astrophysicsatmosphere [showers]Detector alignment and calibration methods (lasers sourcesparticle-beams)FOS: Physical sciencesCosmic rayScintillatorParticle detectorVisible and IR photons (solid-state) (PIN diodes03 medical and health sciencesOpticsSilicon photomultipliermuon: density0103 physical sciencesCalibrationddc:530photomultiplier: silicon[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610High Energy PhysicsCMOS imagersInstrumentation and Methods for Astrophysics (astro-ph.IM)scintillation counterParticle detectors; Detector alignment and calibration methods (lasers sources particle-beams); Photon detectors for UV visible and IR photons (solid-state) (PIN diodes APDs Si-PMTs G-APDs CCDs EBCCDs EMCCDs CMOS imagers etc); Performance of High Energy Physics DetectorsPierre Auger ObservatoryMuonshowers: atmosphere010308 nuclear & particles physicsbusiness.industrymuon: detectorCCDscosmic radiation: primaryDetector alignment and calibration methods (lasersEMCCDsanalog-to-digital converterAPDs; CCDs; CMOS imagers; Detector alignment and calibration methods (lasers; EBCCDs; EMCCDs; Etc); G-APDs; Particle detectors; Particle-beams); Performance of High Energy Physics Detectors; Photon detectors for UV; Si-PMTs; Sources; Visible and IR photons (solid-state) (PIN diodesExperimental High Energy Physicssilicon [photomultiplier]Performance of High Energy Physics DetectorsHigh Energy Physics::Experimentphoton: detectorbusinessalignment [detector]RAIOS CÓSMICOSdetector [photon]astro-ph.IM
researchProduct

GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
researchProduct

Thermal noise limit for ultra-high vacuum noncontact atomic force microscopy

2013

The noise of the frequency-shift signal Δf in noncontact atomic force microscopy (NC-AFM) consists of cantilever thermal noise, tip–surface-interaction noise and instrumental noise from the detection and signal processing systems. We investigate how the displacement-noise spectral density dz at the input of the frequency demodulator propagates to the frequency-shift-noise spectral density dΔf at the demodulator output in dependence of cantilever properties and settings of the signal processing electronics in the limit of a negligible tip–surface interaction and a measurement under ultrahigh-vacuum conditions. For a quantification of the noise figures, we calibrate the cantilever displacemen…

noiseCantilevernoncontact atomic force microscopyGeneral Physics and AstronomyNanotechnologyCantileverlcsh:Chemical technologyNoise (electronics)lcsh:Technology530Full Research PaperOpticsPhase noiseNanotechnologyGeneral Materials ScienceDetection theorylcsh:TP1-1185Electrical and Electronic Engineeringlcsh:SciencePhysicsNoise temperaturefilterbusiness.industrylcsh:TNoise spectral densityBandwidth (signal processing)Spectral density(NC-AFM)noncontact atomic force microscopy (NC-AFM)lcsh:QC1-999Nanosciencelcsh:Qfeedback loopbusinesslcsh:Physics
researchProduct

Modification of a commercial atomic force microscopy for low-noise, high-resolution frequency-modulation imaging in liquid environment.

2011

A key issue for high-resolution frequency-modulation atomic force microscopy imaging in liquids is minimizing the frequency noise, which requires a detailed analysis of the corresponding noise contributions. In this paper, we present a detailed description for modifying a commercial atomic force microscope (Bruker MultiMode V with Nanoscope V controller), aiming at atomic-resolution frequency-modulation imaging in ambient and in liquid environment. Care was taken to maintain the AFMs original stability and ease of operation. The new system builds upon an optimized light source, a new photodiode and an entirely new amplifier. Moreover, we introduce a home-built liquid cell and sample holder …

noiseMaterials scienceoptical sensorsAtomic force acoustic microscopy530Noise (electronics)law.inventionOpticsphotodiodeslawInstrumentationAtomic de Broglie microscopeatomic force microscopycalcium compoundsbusiness.industrysample holdersAmplifierNoise spectral densityPhotodiodefrequency modulationmodulationfrequencyamplifiersbusinessNon-contact atomic force microscopyFrequency modulationimage resolutionThe Review of scientific instruments
researchProduct

Direct Visualization of Molecule Deprotonation on an Insulating Surface

2012

Elucidating molecular-scale details of basic reaction steps on surfaces is decisive for a fundamental understanding of molecular reactivity within many fields, including catalysis and on-surface synthesis. Here, the deprotonation of 2,5-dihydroxybenzoic acid (DHBA) deposited onto calcite (101;4) held at room temperature is followed in situ by noncontact atomic force microscopy. After deposition, the molecules form two coexisting phases, a transient striped phase and a stable dense phase. A detailed analysis of high-resolution noncontact atomic force microscopy images indicates the transient striped phase being a bulk-like phase, which requires hydrogen bonds between the carboxylic acid moie…

noncontact atomic force microscopyCarboxylic acidCatecholsGeneral Physics and AstronomyMicroscopy Atomic ForceKelvin probe force microscopy530Calcium Carbonatechemistry.chemical_compoundDeprotonationPhase (matter)Materials TestingHydroxybenzoatesMoleculeGeneral Materials ScienceReactivity (chemistry)CarboxylateParticle Sizechemistry.chemical_classificationKelvin probe force microscopeHydrogen bondinsulating surfaceGeneral EngineeringElectric ConductivityMolecular ImagingNanostructuresCrystallographychemistrydeprotonationProtons
researchProduct

Mass measurements of As, Se, and Br nuclei, and their implication on the proton-neutron interaction strength toward the N=Z line

2021

Mass measurements of the $^{69}$As, $^{70,71}$Se and $^{71}$Br isotopes, produced via fragmentation of a $^{124}$Xe primary beam at the FRS at GSI, have been performed with the multiple-reflection time-of-flight mass spectrometer (MR-TOF-MS) of the FRS Ion Catcher with an unprecedented mass resolving power of almost 1,000,000. For the $^{69}$As isotope, this is the first direct mass measurement. A mass uncertainty of 22 keV was achieved with only 10 events. For the $^{70}$Se isotope, a mass uncertainty of 2.6 keV was obtained, corresponding to a relative accuracy of $\delta$m/m = 4.0$\times 10^{-8}$, with less than 500 events. The masses of the $^{71}$Se and $^{71}$Br isotopes were measured…

nucl-thNuclear TheoryFOS: Physical sciencesInteraction strengthnucl-exMass spectrometry01 natural sciences7. Clean energyarseeniIonNuclear Theory (nucl-th)Nuclear physicsFragmentation (mass spectrometry)0103 physical sciencesddc:530NeutronbromiNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysicsIsotope010308 nuclear & particles physicsMass measurementAtomic massseleeniydinfysiikkaPhysical Review C
researchProduct

Nuclear mean-square charge radii of $^{63,64,66,68−82}$Ga nuclei: No anomalous behavior at N=32

2012

Collinear laser spectroscopy was performed on the 63,64,66,68−82Ga isotopes with neutron numbers from N = 32 to N = 51. These measurements were carried out at the ISOLDE radioactive ion beam facility at CERN. Here we present the nuclear mean-square charge radii extracted from the isotope shifts and, for the lighter isotopes, new spin and moment values. New ground-state nuclear spin and moments were extracted from the hyperfine spectra of 63,70Ga, measured on an atomic transition in the neutral atom. The ground-state spin of 63Ga is determined to be I = 3/2. Analysis of the trend in the change in mean-square charge radii of the gallium isotopes demonstrates that there is no evidence of anoma…

nuclear spectroscopyydinrakenneaccelerator-based physicsnuclear structureydinspektroskopiaddc:530Physics::Atomic PhysicsNuclear Experimentydinfysiikkakiihdytinpohjainen fysiikka
researchProduct