Search results for "width [Lambda(1405)]"

showing 10 items of 330 documents

First coincidences in pre-clinical Compton camera prototype for medical imaging

2003

Abstract Compton collimated imaging may improve the detection of gamma rays emitted by radioisotopes used in single photon emission computed tomography (SPECT). We present a crude prototype consisting of a single 500 μm thick, 256 pad silicon detector with pad size of 1.4×1.4 mm 2 , combined with a 15×15×1 cm 3 NaI scintillator crystal coupled to a set of 20 photo multipliers. Emphasis is placed on the performance of the silicon detector and the associated read-out electronics, which has so far proved to be the most challenging part of the set-up. Results were obtained using the VATAGP3, 128 channel low-noise self-triggering ASIC as the silicon detector's front-end. The noise distribution (…

PhysicsSingle photon emission computed tomography (SPECT)Nuclear and High Energy PhysicsPhotonbusiness.industryPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGamma rayCompton scatteringScintillatorCollimated lightFull width at half maximum87.58.Ce; 29.40.GxOpticsSilicon pad detectorsCoincidentTracking and position-sensitive detectorsMedical imaging[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]businessInstrumentationNoise (radio)Compton camera
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A Broad Iron Line in the Chandra High Energy Transmission Grating Spectrum of 4U 1705-44

2005

We present the results of a Chandra 30 ks observation of the low-mass X-ray binary and atoll source 4U 1705-44. Here we concentrate on the study of discrete features in the energy spectrum at energies below ~3 keV, as well as on the iron Kalpha line, using the High Energy Transmission Grating Spectrometer on board the Chandra satellite. Below 3 keV, three narrow emission lines are found at 1.47, 2.0, and 2.6 keV. The 1.47 and 2.6 keV lines are probably identified with Lyalpha emission from Mg XII and S XVI, respectively. The identification of the feature at ~2.0 keV is uncertain because of the presence of an instrumental feature at the same energy. The iron Kalpha line at ~6.5 keV is found …

PhysicsSpectrometerAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsaccretion accretion diskstars : individual (4U 1705-44)Coronastars : neutronNeutron starFull width at half maximumSpace and Planetary Scienceindividual (4U 1705-44); stars : neutron; X-rays : binaries; X-rays : general; X-rays : stars [accretion accretion disks; stars]Reflection (physics)Emission spectrumLow MassX-rays : binarieLine (formation)X-rays : general
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A Method Based on Amplitude Probability Density Representation for Sounding High Frequency Noise in Ionospheric Channels

2021

High Frequency (HF) communications efficiency require a precise characterization of the ionospheric channel’s noise. We present a rapid and accurate method to sound the HF ionospheric channels that enables tracing of the time-availability of the channel based on imposed electric field strength thresholds. The method makes use of the amplitude probability density implemented in a real-time spectrum analyzer. Sounding of 3, 10 and 20 kHz bandwidth channels in the 4.8 – 8.8 MHz range is exemplified and specific observations are presented.

PhysicsSpectrum analyzerDepth soundingAmplitudeAcousticsBandwidth (signal processing)Probability density functionNoise (electronics)Communication channelTime–frequency analysis2021 9th International Conference on Modern Power Systems (MPS)
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High Resolution Spectroscopy ofBΛ12by Electroproduction

2007

An experiment measuring electroproduction of hypernuclei has been performed in Hall A at Jefferson Lab on a $^{12}$C target. In order to increase counting rates and provide unambiguous kaon identification two superconducting septum magnets and a Ring Imaging CHerenkov detector (RICH) were added to the Hall A standard equipment. An unprecedented energy resolution of less than 700 keV FWHM has been achieved. Thus, the observed \lam{12}{B} spectrum shows for the first time identifiable strength in the core-excited region between the ground-state {\it s}-wave $\Lambda$ peak and the 11 MeV {\it p}-wave $\Lambda$ peak.

PhysicsSuperconductivity010308 nuclear & particles physicsResolution (electron density)General Physics and AstronomyOrder (ring theory)Lambda01 natural sciencesRing-imaging Cherenkov detectorNuclear physicsFull width at half maximum0103 physical sciencesNuclear Experiment010306 general physicsSpectroscopyEnergy (signal processing)Physical Review Letters
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Pressure tuning of light-induced superconductivity in K3C60

2017

Optical excitation at terahertz frequencies has emerged as an effective means to manipulate complex solids dynamically. In the molecular solid K3C60, coherent excitation of intramolecular vibrations was shown to transform the high temperature metal into a non-equilibrium state with the optical conductivity of a superconductor. Here we tune this effect with hydrostatic pressure, and we find it to disappear around 0.3 GPa. Reduction with pressure underscores the similarity with the equilibrium superconducting phase of K3C60, in which a larger electronic bandwidth is detrimental for pairing. Crucially, our observation excludes alternative interpretations based on a high-mobility metallic phase…

PhysicsSuperconductivityCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Terahertz radiationCondensed Matter - SuperconductivityBandwidth (signal processing)Hydrostatic pressureGeneral Physics and AstronomyFOS: Physical sciences02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesArticleSuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsMolecular solidPairingCondensed Matter::Superconductivity0103 physical sciencesPressure tuning010306 general physics0210 nano-technologyExcitationNature physics
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Calibration of the NEXT-White detector using 83m Kr decays

2018

The NEXT-White (NEW) detector is currently the largest radio-pure high-pressure xenon gas time projection chamber with electroluminescent readout in the world. It has been operating at Laboratorio Subterr'aneo de Canfranc (LSC) since October 2016. This paper describes the calibrations performed using 83mKr decays during a long run taken from March to November 2017 (Run II). Krypton calibrations are used to correct for the finite drift-electron lifetime as well as for the dependence of the measured energy on the event transverse position which is caused by variations in solid angle coverage both for direct and reflected light and edge effects. After producing calibration maps to correct for …

PhysicsTime projection chamber010308 nuclear & particles physicsKryptonDetectorSolid anglechemistry.chemical_element01 natural sciencesNuclear physicsFull width at half maximumXenonchemistryDouble beta decay0103 physical sciencesCalibration010306 general physicsInstrumentationMathematical PhysicsJournal of Instrumentation
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Inverse dispersion engineering in silicon waveguides

2014

We present a numerical tool that searches an optimal cross section geometry of silicon-on-insulator waveguides given a target dispersion profile. The approach is a gradient-based multidimensional method whose efficiency resides on the simultaneous calculation of the propagation constant derivatives with respect to all geometrical parameters of the structure by using the waveguide mode distribution. The algorithm is compatible with regular mode solvers. As an illustrative example, using a silicon slot hybrid waveguide with 4 independent degrees of freedom, our approach finds ultra-flattened (either normal or anomalous) dispersion over 350 nm bandwidth in less than 10 iterations.

PhysicsWaveguide (electromagnetism)Siliconbusiness.industryBandwidth (signal processing)Mathematical analysischemistry.chemical_elementInverseStatistical and Nonlinear PhysicsÒpticaAtomic and Molecular Physics and OpticsNonlinear systemOpticschemistryPropagation constantbusinessRefractive indexPhotonic-crystal fiber
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Development of the wide field imager for Athena

2015

The WFI (Wide Field Imager) instrument is planned to be one of two complementary focal plane cameras on ESA's next X-ray observatory Athena. It combines unprecedented survey power through its large field of view of 40 arcmin x 40 arcmin together with excellent count-rate capability (>= 1 Crab). The energy resolution of the silicon sensor is state-of-the-art in the energy band of interest from 0.2 keV to 15 keV, e.g. the full width at half maximum of a line at 6 keV will be <= 150 eV until the end of the nominal mission phase. This performance is accomplished by using DEPFET active pixel sensors with a pixel size of 130 μm x 130 μm well suited to the on-axis angular resolution of 5 arcsec of…

PhysicsX-ray detectorCMOS sensorHot and Energetic UniversePixelbusiness.industryElectronic Optical and Magnetic MaterialApplied MathematicsX-ray detectorComputer Science Applications1707 Computer Vision and Pattern Recognitionfocal plane cameraCondensed Matter PhysicX-ray astronomyFull width at half maximumCardinal pointOpticsActive pixel sensorObservatoryWFIAngular resolutionAthenaElectrical and Electronic EngineeringbusinessImage resolutionDEPFET
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X-ray spectroscopy and dosimetry with a portable CdTe device.

2007

Abstract X-ray spectra and dosimetry information are very important for quality assurance (QA) and quality control (QC) in medical diagnostic X-ray systems. An accurate knowledge of the diagnostic X-ray spectra would improve the patient dose optimization, without compromising image information. In this work, we performed direct diagnostic X-ray spectra measurements with a portable device, based on a CdTe solid-state detector. The portable device is able to directly measure X-ray spectra at high photon fluence rates, as typical of clinical radiography. We investigated on the spectral performances of the system in the mammographic energy range (up to ∼40 keV). Good system response to monoener…

PhysicsX-ray spectroscopy CdTe detectorsNuclear and High Energy Physicsmedicine.medical_specialtyReproducibilitybusiness.industryDetectorExposure HVLFluenceFull width at half maximumQuality (physics)OpticsmedicineDosimetryMedical physicsSpectroscopybusinessInstrumentationHalf-value layer
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Characterization of Al-Schottky CdTe detectors

2011

In the last decades, great efforts are being devoted to the development of CdTe detectors for high resolution X-ray and gamma ray spectroscopy. Recently, new rectifying contacts based on aluminum (Al) are very appealing in the development of CdTe detectors with low leakage currents and anode pixellization. In this work, we report on preliminary results of electrical and spectroscopic investigations on Schottky CdTe diode detectors (4.1 × 4.1 × 0.75 and 4.1 × 4.1 × 2 mm3) with Au/Ti/Al/CdTe/Pt electrode configuration. The detectors are characterized by very low leakage currents even at room temperature (26 pA at 25 °C under a bias voltage of −100 V for the 2 mm thick detector). Polarization …

PhysicsX-ray spectroscopySpectrometerbusiness.industrySettore FIS/01 - Fisica SperimentaleDetectorSchottky diodeBiasingSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)AnodeCdTe detectorFull width at half maximumX-ray and gamma ray spectroscopyOpticsOptoelectronicsGamma spectroscopybusiness2011 IEEE Nuclear Science Symposium Conference Record
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