Search results for "Instrumentation"

showing 10 items of 4914 documents

Spectral broadening by incomplete thermalization of the energy in X-ray microcalorimeters with superconducting absorber and NTD-Ge thermal sensor

2004

Abstract We present a model of the response of a cryogenic microcalorimeter with superconducting absorber and phonon sensitive thermal sensor to the absorption of X-ray photons. The model is based on the main microscopic processes responsible for the thermalization of the deposited energy. We use a system of rate equations to describe the energy downconversion in the superconductor and transport to the thermal sensor. The model is a tool to investigate the thermalization efficiency with respect to the device characteristics (i.e. absorber material, geometry), in order to optimize the performances of these detectors. As a first case study, we report results of simulations for a microcalorime…

PhysicsSuperconductivityquasi-particleNuclear and High Energy PhysicsPhotonbusiness.industryPhononx-ray spectroscopymicrocalorimeterParticle detectorgermaniumThermalisationOpticsCondensed Matter::Superconductivitynumerical simulationNeutronAtomic physicsAbsorption (electromagnetic radiation)businessInstrumentationDoppler broadening
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Estimate of the gravitational-wave background from the observed cosmological distribution of quasars

2021

We study the gravitational-wave background from the observed cosmological quasar distribution. Using the DR9Q quasar catalogue from the ninth data release of the Sloan Digital Sky Survey (SDSS), we create a complete, statistically consistent sample of quasars from $z=0.3$ to $5.4$. Employing the spectroscopic information from the catalogue we estimate the masses of the supermassive black holes hosted by the quasars in the sample, resulting in a log-normal distribution of mean $10^{8.32\pm0.33}M_{\odot}$. The computation of the individual gravitational-wave strains relies on specific functional forms derived from simulations of gravitational collapse and mergers of massive black hole binarie…

PhysicsSupermassive black hole010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectAstrophysics::Instrumentation and Methods for AstrophysicsPlane waveFOS: Physical sciencesQuasarGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational wave backgroundBlack holeGeneral Relativity and Quantum CosmologyDistribution (mathematics)Sky0103 physical sciencesGravitational collapse010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonPhysical Review D
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IceCube Sensitivity for Low-Energy Neutrinos from Nearby Supernovae ( Corrigendum )

2014

Keywords: neutrinos ; supernovae: general ; instrumentation: detectors ; errata ; addenda Reference EPFL-ARTICLE-198916doi:10.1051/0004-6361/201117810eView record in Web of Science Record created on 2014-05-19, modified on 2017-05-12

PhysicsSupernovaLow energyWeb of scienceSpace and Planetary Scienceddc:520Astronomy and AstrophysicsAstrophysicsInstrumentation (computer programming)Sensitivity (control systems)Neutrino
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Geometric efficiency for a parallel-surface source and detector system with at least one axisymmetric surface

2007

Abstract An exact and numerically friendly method is given to calculate the geometric efficiency G of a planar radiation source and cosine detector system. Either the source or the detector, but not necessarily both, must have axial symmetry. For two non-coaxial disks the results are in exact agreement with a recent generalization of Ruby's formula for G. Detailed formulas and sample numerical results are given for a disk combined with rectangles and triangles. A disk and a general polygon can be solved by dividing the polygon into triangles. The method can also be applied to electrical inductance calculations and a solution recently given for the inductance of circular and elliptic loops c…

PhysicsSurface (mathematics)Nuclear and High Energy PhysicsMathematical analysisDetectorPolygonSolid angleRotational symmetryTrigonometric functionsElliptic integralAxial symmetryInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Reduction of the uncertainty in the measurements of magnetic fields

2014

The paper deals with magnetic field measurement, carried out by using a broadband and isotropic instrument. These measurements are characterized by a very high uncertainty values if compared with the ones usually related to other electrical measurements. For these reasons, if the measurements are performed to assess the exposure of human beings, these large uncertainty values imply a high risk of wrong decision when there is the need to establish if a site complies or does not comply with a specified emission limits. A reduction of the uncertainty values implies a reduction of the risk. With this aim, we propose an approach which, in particular but very typical cases, allows an effective re…

PhysicsSustainability and the EnvironmentMagnetoresistancebusiness.industrymagnetic field measurementsIsotropyElectrical engineeringmeasurement uncertainty.Magnetic fieldReduction (complexity)Control theorymagnetic field measurementmeasurement uncertaintyCalibrationSettore ING-IND/09 - Sistemi per l'Energia e L'AmbienteMeasurement uncertaintyElectrical measurementsRenewable EnergyInstrumentation (computer programming)businessSettore ING-INF/07 - Misure Elettriche E Elettronichemagnetic field measurements; measurement uncertainty; Renewable Energy Sustainability and the Environment2014 International Conference on Renewable Energy Research and Application (ICRERA)
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The Status of the Ultra Fast Flash Observatory - Pathfinder

2012

On behalf of the UFFO Collaboration; International audience; The Ultra Fast Flash Observatory (UFFO) is a project to study early optical emissions from Gamma Ray Bursts (GRBs). The primary scientific goal of UFFO is to see if GRBs can be calibrated with their rising times, so that they could be used as new standard candles. In order to minimize delay in optical follow-up measurements, which is now about 100 sec after trigger from the Swift experiment, we rotate a mirror to redirect light path so that optical measurement can be performed within a second after the trigger. We have developed a pathfinder mission, UFFO-pathfinder to launch on board the Lomonosov satellite in 2012. In this talk,…

PhysicsSwiftNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyCosmic ray01 natural sciencesAtomic and Molecular Physics and OpticsEarly Light Emissions[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Flash (photography)PathfinderObservatory0103 physical sciencesGamma Ray BurstsUltra fastSatelliteGamma-ray burst010303 astronomy & astrophysicscomputerUltra Fast Flash Observatorycomputer.programming_language
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Laser cooling of externally produced Mg ions in a Penning trap for sympathetic cooling of highly charged ions

2012

We have performed laser cooling of Mg ions confined in a Penning trap. The externally produced ions were captured in flight, stored and laser cooled. Laser-induced fluorescence was observed perpendicular to the cooling laser axis. Optical detection down to the single ion level together with electronic detection of the ion oscillations inside the Penning trap have been used to acquire information on the ion storage time, ion number and ion temperature. Evidence for formation of ion crystals has been observed. These investigations are an important prerequisite for sympathetic cooling of simultaneously stored highly-charged ions and precision laser spectroscopy of forbidden transitions in thes…

PhysicsSympathetic coolingPhysics - Instrumentation and DetectorsAtomic Physics (physics.atom-ph)FOS: Physical sciencesPhysics::OpticsInstrumentation and Detectors (physics.ins-det)Penning trapLaserIon trappingAtomic and Molecular Physics and OpticsIonlaw.inventionPhysics - Atomic PhysicslawPhysics::Plasma PhysicsLaser coolingIon trapPhysics::Atomic PhysicsAtomic physicsSpectroscopy
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Estimating the magnetic moment of microscopic magnetic sources from their magnetic field distribution in a layer of nitrogen-vacancy (NV) centres in …

2016

We have used a synthetic diamond with a layer of nitrogen-vacancy (NV) centres to image the magnetic field distributions of magnetic particles on the surface of the diamond. Magnetic field distributions of 4 µ m and 2 µ m ferromagnetic and 500 nm diameter superparamagnetic particles were obtained by measuring the position of the optically detected magnetic resonance peak in the fluorescence emitted by the NV centres for each pixel. We fitted the results to a model in order to determine the magnetic moment of the particles from the magnetic field image and compared the results to the measured magnetic moment of the particles. The best-fit magnetic moment differed from the value expected base…

PhysicsSynthetic diamondCondensed matter physicsMagnetic momentMagnetometerDiamond02 engineering and technologyengineering.material021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesElectronic Optical and Magnetic Materialslaw.inventionMagnetic fieldNuclear magnetic resonanceFerromagnetismlaw0103 physical sciencesengineeringMagnetic nanoparticles010306 general physics0210 nano-technologyInstrumentationSuperparamagnetismThe European Physical Journal Applied Physics
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Analysis and calibration of absorptive images of Bose-Einstein condensate at non-zero temperatures

2008

We describe the method allowing quantitative interpretation of absorptive images of mixtures of BEC and thermal atoms which reduces possible systematic errors associated with evaluation of the contribution of each fraction. By using known temperature dependence of the BEC fraction, the analysis allows precise calibration of the fitting results. The developed method is verified in two different measurements and compares well with theoretical calculations and with measurements performed by another group.

PhysicsSystematic errorCondensed Matter::Quantum GasesZero (complex analysis)FOS: Physical sciencesInterpretation (model theory)Computational physicslaw.inventionCondensed Matter - Other Condensed MatterlawThermalCalibrationFraction (mathematics)InstrumentationBose–Einstein condensateOther Condensed Matter (cond-mat.other)
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New methods of evaluation of the flavor composition in e+ e- annihilation by double hemisphere tagging at LEP / SLC energies

1995

Two new methods are proposed to extract the flavour contents of the events produced at LEP/SLC, together with the classification matrix of a tagging by hemispheres. By utilising the tagging obtained in both hemispheres, the efficiencies, backgrounds and flavour compositions are directly obtained by fitting the data. A minimal dependence on modelling and a consistent treatment of systematic errors are achieved by applying these methods. The choice of the tagging algorithm is irrelevant in the methods, provided that similar efficiencies are reached. As an example, a multivariate analysis technique combining the tracking information given by a microvertex detector has been applied to extract t…

PhysicsSystematic errorNuclear and High Energy PhysicsAnnihilationBranching fractionFlavourDetectorHigh Energy Physics::PhenomenologyComposition (combinatorics)Tracking (particle physics)Nuclear physicsMatrix (mathematics)Física nuclearHigh Energy Physics::ExperimentDetectors and Experimental TechniquesInstrumentation
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