Search results for "design [semiconductor detector]"

showing 10 items of 613 documents

A Comparison of Multi-objective Algorithms for the Automatic Design Space Exploration of a Superscalar System

2013

In today’s computer architectures the design spaces are huge, thus making it very difficult to find optimal configurations. One way to cope with this problem is to use Automatic Design Space Exploration (ADSE) techniques. We developed the Framework for Automatic Design Space Exploration (FADSE) which is focused on microarchitectural optimizations. This framework includes several state-of-the art heuristic algorithms.

Heuristic (computer science)Design space explorationComputer scienceSuperscalarParticle swarm optimizationAlgorithm
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Spectral analysis of the low-mass X-ray pulsar 4U 1822-371: Reflection component in a high-inclination system

2021

Context. The X-ray source 4U 1822-371 is an eclipsing low-mass X-ray binary and X-ray pulsar, hosting a NS that shows periodic pulsations in the X-ray band with a period of 0.59 s. The inclination angle of the system is so high (80–85°) that in principle, it should be hard to observe both the direct thermal emission of the central object and the reflection component of the spectrum because they are hidden by the outer edge of the accretion disc. Despite the number of studies carried out on this source, many aspects such as the geometry of the system, its luminosity, and its spectral features are still debated. Aims. Assuming that the source accretes at the Eddington limit, the analysis perf…

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsRadiusAstrophysics01 natural sciencesaccretion accretion disks stars: neutron stars: individual: 4U 1822-371 X-rays: binaries X-rays: general eclipsesLuminositysymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary Science0103 physical sciencesEddington luminosityReflection (physics)symbolsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsX-ray pulsarEclipse
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Magneto-elastic oscillations of neutron stars: exploring different magnetic field configurations

2012

We study magneto-elastic oscillations of highly magnetized neutron stars (magnetars) which have been proposed as an explanation for the quasi-periodic oscillations (QPOs) appearing in the decaying tail of the giant flares of soft gamma-ray repeaters (SGRs). We extend previous studies by investigating various magnetic field configurations, computing the Alfv��n spectrum in each case and performing magneto-elastic simulations for a selected number of models. By identifying the observed frequencies of 28 Hz (SGR 1900+14) and 30 Hz (SGR 1806-20) with the fundamental Alfv��n QPOs, we estimate the required surface magnetic field strength. For the magnetic field configurations investigated (dipole…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsField lineAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsMagnetar01 natural sciencesAsteroseismologyGeneral Relativity and Quantum CosmologyMagnetic fieldDipoleNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamics010306 general physicsAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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Radio emission of SN1993J. The complete picture: II. Simultaneous fit of expansion and radio light curves

2010

We report on a simultaneous modelling of the expansion and radio light curves of SN1993J. We have developed a simulation code capable of generating synthetic expansion and radio light curves of supernovae by taking into consideration the evolution of the expanding shock, magnetic fields, and relativistic electrons, as well as the finite sensitivity of the interferometric arrays used in the observations. Our software successfully fits all the available radio data of SN 1993J with an standard emission model for supernovae extended with some physical considerations, as an evolution in the opacity of the ejecta material, a radial drop of the magnetic fields inside the radiating region, and a ch…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsOpacityAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLight curveGalaxyMagnetic fieldParticle accelerationSupernovaSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsEjectaAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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Testing Rate Dependent corrections on timing mode EPIC-pn spectra of the accreting Neutron Star GX 13+1

2014

When the EPIC-pn instrument on board XMM-Newton is operated in Timing mode, high count rates (>100 cts/s) of bright sources may affect the calibration of the energy scale, resulting in a modification of the real spectral shape. The corrections related to this effect are then strongly important in the study of the spectral properties. Tests of these calibrations are more suitable in sources which spectra are characterised by a large number of discrete features. Therefore, in this work, we carried out a spectral analysis of the accreting Neutron Star GX 13+1, which is a dipping source with several narrow absorption lines and a broad emission line in its spectrum. We tested two different co…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion discs line: identification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1)Spectral shape analysisAccretion (meteorology)Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesSpectral lineNeutron starAmplitudeidentification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1) [accretion accretion discs line]Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Emission spectrumAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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Sensitivity of one-neutron knockout of halo nuclei to their nuclear structure

2019

Halo nuclei are located far from stability and exhibit a very peculiar structure. Due to their very short lifetime, they are often studied through reactions. Breakup reactions are of particular interest since their cross sections are large for these loosely-bound nuclei. Inclusive measurements of breakup--also called knockout reactions--have even higher statistics. In this proceeding, we study which nuclear-structure information can be inferred from the parallel-momentum distribution of the core of one-neutron halo nuclei after the knockout of its halo neutron. In particular, we analyse the influence of the ground-state wavefunction, the presence of excited states within the halo-nucleus sp…

HistoryNuclear TheoryContinuum (design consultancy)Nuclear TheoryFOS: Physical sciences01 natural sciencesEducationNuclear Theory (nucl-th)Nuclear physics0103 physical sciencesNeutronNuclear Experiment (nucl-ex)010306 general physicsWave functionNuclear ExperimentNuclear ExperimentPhysicsPhysique010308 nuclear & particles physicsNuclear structureObservableAstronomieBreakupComputer Science ApplicationsExcited stateHalo
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Studio delle prestazioni di giunzioni incollate ibride

2011

Le giunzioni ibride sono giunzioni in cui coesistono due differenti tipologie di giunzione, di cui una è l’incollaggio. L’articolo mostra i risultati di una campagna sperimentale volta a caratterizzare le prestazioni di giunti incollati ibridi in confronto ad alcune tipologie di giunzioni tradizionali. Si sono prese in considerazioni come tecnologie di giunzione tradizionali la saldatura a resistenza, la rivettatura a strappo, la clinciatura e la rivettatura auto perforante. In particolare si sono studiate le prestazioni di giunti a semplice sovrapposizione per differenti condizioni geometriche del giunto (spessore aderendi, passo tra i punti di fissaggio meccanico) e condizioni ambientali …

Hybrid JoiningAdhesive Bondinglcsh:Mechanical engineering and machinerylcsh:TA630-695lcsh:TJ1-1570lcsh:Structural engineering (General)Design of ExperimentFrattura ed Integrità Strutturale
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New Cathepsin Inhibitors to Explore the Fluorophilic Properties of the S 2 Pocket of Cathepsin B: Design, Synthesis, and Biological Evaluation

2011

5 páginas, 1 figura, 2 tablas -- PAGS nros. 5256-5260

Hydrocarbons FluorinatedStereochemistryStereoisomerismhydrolasesstereoselectivityCatalysisCathepsin BCathepsin BNitrilesinhibitorsCombinatorial Chemistry TechniquesHumansMoleculefluorinated ligandsBiological evaluationCathepsinMolecular StructureCombinatorial Chemistry TechniquesligandsChemistryOrganic ChemistryStereoisomerismDipeptidesGeneral Chemistryfluorinated fluorinatedDesign synthesisDrug DesignpeptidesStereoselectivityChemistry – A European Journal
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Aspects of values in human-technology interaction design : a content-based view to values

2011

ICT-ethicsmental contentsvuorovaikutusInformation Societymental representationshuman-technology interactionHTIdesign thinkingvaluesteknologiaICT-etiikkacontent-based approachihminenarvotetiikkasisältöperustainen lähestymistapa
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In vitro evaluation of poloxamer in situ forming gels for bedaquiline fumarate salt and pharmacokinetics following intramuscular injection in rats

2019

Graphical abstract

In situPO Propylene oxideIV IntravenousP338 Poloxamer 338lcsh:RS1-441Pharmaceutical Sciencechemistry.chemical_compoundn Sample sizeSD Standard deviationIM Intramuscularchemistry.chemical_classificationC0 Analyte plasma concentration at time zeroDoE Design of experimentsUV UltravioletPharmacology. TherapyK2.EDTA Potassium ethylenediaminetetraacetic acidLC–MS/MS Liquid chromatography-tandem mass spectrometryH&E Hematoxylin and eosintmax Sampling time to reach the maximum observed analyte plasma concentrationIn situ forming gelsCMC Critical micellar concentrationCmax Maximum observed analyte plasma concentrationIntramuscular injectionDN Dose normalizedGPT Gel point temperaturePLGA Poly-(DL-lactic-co-glycolic acid)TFA Trifluoroacetic acidCAN AcetonitrileATP Adenosine 5′ triphosphateSalt (chemistry)Polyethylene glycolPoloxamerArticlelcsh:Pharmacy and materia medicaPharmacokineticsIn vivoUHPLC Ultra-high performance liquid chromatographyPharmacokineticsAUClast Area under the analyte concentration versus time curve from time zero to the time of the last measurable (non-below quantification level) concentrationEO Ethylene oxideNMP N-methyl-2-pyrrolidoneComputingMethodologies_COMPUTERGRAPHICSAUC∞ Area under the analyte concentration vs time curve from time zero to infinite timeP407 Poloxamer 407In vitro releasePoloxamerCMT Critical micellar temperatureGel erosionIn vitrot1/2 Apparent terminal elimination half-lifechemistryMDR-TB Multi-drug resistant tuberculosisAUC80h Area under the analyte concentration versus time curve from time zero to 80 htlast Sampling time until the last measurable (non-below quantification level) analyte plasma concentrationMRM Multiple reaction monitoringNuclear chemistrySustained releaseInternational Journal of Pharmaceutics: X
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