Search results for " Instrumentation."

showing 10 items of 712 documents

Comparison of different methods for evaluating the transmission function of a two-stage cylindrical mirror analizer in XPS applications

2007

Three different evaluations of the energy dependence of the transmission-detection function of a two-stage cylindrical electron analyzer have been obtained by resorting to three established procedures. Their relative merits have been tested as follows. First they have been used to correct raw XPS spectra of clean Cu, Ag and Au surfaces. Next, the secondary electron background has been subtracted using Tougaard's method. Finally, the primary electron spectra so obtained have been reanalyzed by peak area measurement in the frame of the modern formalism for quantitative XPS analysis. Ideally a constant residual value should thus be obtained. The variability of these residuals with peak energy …

Physics - Instrumentation and Detectorstwo-stage CMAtransmission function[ SPI.MAT ] Engineering Sciences [physics]/MaterialsXPSFOS: Physical sciencescylindrical mirror analyzer[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Detectors (physics.ins-det)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][SPI.MAT]Engineering Sciences [physics]/Materials
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Search for Electronic Recoil Event Rate Modulation with 4 Years of XENON100 Data

2017

We report on a search for electronic recoil event rate modulation signatures in the XENON100 data accumulated over a period of 4 years, from January 2010 to January 2014. A profile likelihood method, which incorporates the stability of the XENON100 detector and the known electronic recoil background model, is used to quantify the significance of periodicity in the time distribution of events. There is a weak modulation signature at a period of $431^{+16}_{-14}$ days in the low energy region of $(2.0-5.8)$ keV in the single scatter event sample, with a global significance of $1.9\,\sigma$, however no other more significant modulation is observed. The expected annual modulation of a dark matt…

Physics and Astronomy (all) XENON DARK MATTER MODULATION TPCPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterGeneral Physics and AstronomyFOS: Physical sciencesElectron01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Recoil0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPseudovectorInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)Coupling (probability)ModulationAstrophysics - Instrumentation and Methods for AstrophysicsEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics
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A method for approximating optimal statistical significances with machine-learned likelihoods

2022

The European physical journal / C 82(11), 993 (2022). doi:10.1140/epjc/s10052-022-10944-3

Physics and Astronomy (miscellaneous)Gluonsboosted particleFOS: Physical sciencesTop Quark530High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)statistical analysisddc:530numerical calculationsEngineering (miscellaneous)Monte CarloInstrumentation and Methods for Astrophysics (astro-ph.IM)new physicsFísicadijet: final statefinal state [dijet]sensitivityHigh Energy Physics - Phenomenologymachine learningCERN LHC CollPhysics - Data Analysis Statistics and ProbabilitySubstructureAstrophysics - Instrumentation and Methods for AstrophysicsData Analysis Statistics and Probability (physics.data-an)
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Classification of gravitational-wave glitches via dictionary learning

2018

We present a new method for the classification of transient noise signals (or glitches) in advanced gravitational-wave interferometers. The method uses learned dictionaries (a supervised machine learning algorithm) for signal denoising, and untrained dictionaries for the final sparse reconstruction and classification. We use a data set of 3000 simulated glitches of three different waveform morphologies, comprising 1000 glitches per morphology. These data are embedded in non-white Gaussian noise to simulate the background noise of advanced LIGO in its broadband configuration. Our classification method yields a 96% accuracy for a large range of initial parameters, showing that learned diction…

Physics and Astronomy (miscellaneous)Noise reductionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Data_CODINGANDINFORMATIONTHEORY01 natural sciencesGeneral Relativity and Quantum CosmologyBackground noiseTransient noisesymbols.namesake0103 physical sciencesWaveformAstrophysics::Solar and Stellar Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPattern recognitionLIGOGlitchGaussian noisesymbolsArtificial intelligenceAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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New method to observe gravitational waves emitted by core collapse supernovae

2018

While gravitational waves have been detected from mergers of binary black holes and binary neutron stars, signals from core collapse supernovae, the most energetic explosions in the modern Universe, have not been detected yet. Here we present a new method to analyse the data of the LIGO, Virgo, and KAGRA network to enhance the detection efficiency of this category of signals. The method takes advantage of a peculiarity of the gravitational wave signal emitted in the core collapse supernova and it is based on a classification procedure of the time-frequency images of the network data performed by a convolutional neural network trained to perform the task to recognize the signal. We validate …

Physics010308 nuclear & particles physicsGravitational waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsType II supernova01 natural sciencesSignalGeneral Relativity and Quantum CosmologyLIGOGravitational wavesGravitational waves; SupernovaeGeneral Relativity and Quantum CosmologySupernovaNeutron starSupernovaeBinary black hole0103 physical sciencesKAGRAAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics
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Total-variation methods for gravitational-wave denoising: Performance tests on Advanced LIGO data

2018

We assess total-variation methods to denoise gravitational-wave signals in real noise conditions, by injecting numerical-relativity waveforms from core-collapse supernovae and binary black hole mergers in data from the first observing run of Advanced LIGO. This work is an extension of our previous investigation where only Gaussian noise was used. Since the quality of the results depends on the regularization parameter of the model, we perform an heuristic search for the value that produces the best results. We discuss various approaches for the selection of this parameter, either based on the optimal, mean, or multiple values, and compare the results of the denoising upon these choices. Mor…

PhysicsArtificial neural network010308 nuclear & particles physicsGravitational waveNoise reductionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLIGOsymbols.namesakeAstrophysics - Solar and Stellar AstrophysicsBinary black holeGaussian noiseLagrange multiplier0103 physical sciencessymbolsWaveformAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)AlgorithmSolar and Stellar Astrophysics (astro-ph.SR)Physical Review D
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Characterization of a Be(p,xn) Neutron Source for Fission Yields Measurements

2013

We report on measurements performed at The Svedberg Laboratory (TSL) to characterize a proton-neutron converter for independent fission yield studies at the IGISOL-JYFLTRAP facility (Jyv\"askyl\"a, Finland). A 30 MeV proton beam impinged on a 5 mm water-cooled Beryllium target. Two independent experimental techniques have been used to measure the neutron spectrum: a Time of Flight (TOF) system used to estimate the high-energy contribution, and a Bonner Sphere Spectrometer able to provide precise results from thermal energies up to 20 MeV. An overlap between the energy regions covered by the two systems will permit a cross-check of the results from the different techniques. In this paper, th…

PhysicsBonner sphereNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsSpectrometerta114010308 nuclear & particles physicsFissionNuclear TheoryNuclear dataFOS: Physical sciencesFission product yieldInstrumentation and Detectors (physics.ins-det)7. Clean energy01 natural sciencesThe Svedberg LaboratoryNuclear physics0103 physical sciencesNeutron sourceNeutronNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentNuclear ExperimentNuclear Data Sheets
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Toward early-warning detection of gravitational waves from compact binary coalescence

2012

Rapid detection of compact binary coalescence (CBC) with a network of advanced gravitational-wave detectors will offer a unique opportunity for multi-messenger astronomy. Prompt detection alerts for the astronomical community might make it possible to observe the onset of electromagnetic emission from (CBC). We demonstrate a computationally practical filtering strategy that could produce early-warning triggers before gravitational radiation from the final merger has arrived at the detectors.

PhysicsCoalescence (physics)Warning system010308 nuclear & particles physicsGravitational waveDetectorAstronomyBinary numberFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Electromagnetic emission01 natural sciencesRapid detectionGeneral Relativity and Quantum CosmologySpace and Planetary Science0103 physical sciencesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Computer Science::Cryptography and Security
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Band structure tuning of Heusler compounds: Spin- and momentum-resolved electronic structure analysis of compounds with different band filling

2019

Physical review / B 103(5), 054407 (2021). doi:10.1103/PhysRevB.103.054407

PhysicsCondensed Matter - Materials SciencePhysics - Instrumentation and DetectorsValence (chemistry)Band gapPhotoemission spectroscopyMagnetismMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciences02 engineering and technologyElectronic structureInstrumentation and Detectors (physics.ins-det)021001 nanoscience & nanotechnology01 natural sciences530Brillouin zoneCrystallographyFerromagnetism0103 physical sciencesddc:530Condensed Matter::Strongly Correlated Electrons010306 general physics0210 nano-technologyElectronic band structureValence electron
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Cosmic magnetic fields with masclet: an application to galaxy clusters

2020

We describe and test a new version of the adaptive mesh refinement (AMR) cosmological code MASCLET. The new version of the code includes all the ingredients of its previous version plus a description of the evolution of the magnetic field under the approximation of the ideal magneto-hydrodynamics (MHD). To preserve the divergence-free condition of MHD, the original divergence cleaning algorithm of Dedner et al. (2002) is implemented. We present a set of well-known 1D and 2D tests, such as several shock-tube problems, the fast rotor and the Orszag-Tang vortex. The performance of the code in all the tests is excellent with estimated median relative errors of $\nabla \cdot {\bf B}$ in the 2D t…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Adaptive mesh refinementFOS: Physical sciencesOrder (ring theory)Astronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsMagnetic fieldComputational physicsVortexSpace and Planetary ScienceGalaxy formation and evolutionNabla symbolMagnetohydrodynamicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Galaxy clusterAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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