Search results for "Instrumentation"

showing 10 items of 4914 documents

Decoherent neutrino mixing, dark energy, and matter-antimatter asymmetry

2004

A CPT violating decoherence scenario can easily account for all the experimental evidence in the neutrino sector including LSND. In this work it is argued that this framework can also accommodate the Dark Energy content of the Universe, as well as the observed matter-antimatter asymmetry.

High Energy Physics - TheoryPhysics::General PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsCPT symmetrymedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Neutrino oscillationComputer Science::Databasesmedia_commonPhysicsHigh Energy Physics::PhenomenologyFísicaUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Neutrino detectorAntimatterDark energyHigh Energy Physics::ExperimentNeutrinoPhysical Review D
researchProduct

Foreground Contributions to 0.2-2 Degree CMB Anisotropies

1994

We examine the extent to which galactic and extragalactic foregrounds can hamper the detection of primordial Cosmic Microwave Background (CMB) anisotropies. We limit our discussion to intermediate angular scales, $10^{\prime}\lsim \theta \lsim 2^{\circ}$, since many current as well as future experiments have been designed to map CMB anisotropies at these angular scales. In fact, scales of $\gsim 10^{\prime}$ are of crucial importance to test both the conditions in the early Universe and current theories of the gravitational collapse.

High Energy Physics::PhenomenologyAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysics::Galaxy Astrophysics
researchProduct

IAXO - The International Axion Observatory

2013

The International Axion Observatory (IAXO) is a next generation axion helioscope aiming at a sensitivity to the axion-photon coupling of a few 10^{-12} GeV^{-1}, i.e. 1-1.5 orders of magnitude beyond sensitivities achieved by the currently most sensitive axion helioscope, the CERN Axion Solar Telescope (CAST). Crucial factors in improving the sensitivity for IAXO are the increase of the magnetic field volume together with the extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested at CAST. Electron-coupled axions invoked to explain the white dwarf cooling, relic axions, and a large variety of more generic axion-like particles (ALPs) along…

High Energy Physics::TheoryHigh Energy Physics - Experiment (hep-ex)Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Detectors and Experimental TechniquesHigh Energy Physics - Experiment
researchProduct

Streuung von mittelschnellen Elektronen an Kunststoff-Folien mit eingelagerten Schwermetallatomen

1962

Scattering has been observed of 70-keV electrons by Kollodium-foils containing elements of high atomic number (lead). The contents of lead are determined and the kind of distribution of lead in the foil is described. The differential cross-section as a function of the angle of scattering approximates the cross-section calculated by Sherman with lower contents of lead of the foils. Remaining deviations can be explained by screening-effects of the electron cloud.

High atomic numberPhysicsNuclear and High Energy PhysicsAtomic orbitalPhysics::Instrumentation and DetectorsScatteringNuclear fusionElectronAtomic physicsFOIL methodZeitschrift f�r Physik
researchProduct

Intrinsic defects induced by β-irradiation in silica

2002

We report an electron paramagnetic resonance study of defects induced by β-irradiation in natural and synthetic samples of high purity commercial silica. Data are collected for the E′ centers and a resonance satellite signal split by 1.36 mT. By comparison with the effects of γ-irradiation it is shown that the mechanisms of defect generation are the same for the two irradiation sources and that in the high-dose limit they involve intrinsic defects of the glassy matrix. Moreover, the high concentration of defects generated by β-irradiation modifies the EPR spectrum due to spin–spin interaction.

High concentrationNuclear and High Energy PhysicsMaterials sciencePhysics::Medical Physicsβ irradiationResonancePhotochemistryCrystallographic defectlaw.inventionNuclear magnetic resonancelawGlassy matrixIrradiationElectron paramagnetic resonanceInstrumentationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
researchProduct

Initial results on energy resolution of the NEXT-White detector

2018

One of the major goals of the NEXT-White (NEW) detector is to demonstrate the energy resolution that an electroluminescent high pressure xenon TPC can achieve for high energy tracks. For this purpose, energy calibrations with 137Cs and 232Th sources have been carried out as a part of the long run taken with the detector during most of 2017. This paper describes the initial results obtained with those calibrations, showing excellent linearity and an energy resolution that extrapolates to approximately 1% FWHM at Q$_{\beta\beta}$.

High energyPhysics - Instrumentation and DetectorsTime projection chamberschemistry.chemical_elementFOS: Physical sciences01 natural sciencesXenonOpticsEngineeringAffordable and Clean Energy0103 physical sciences010306 general physicsInstrumentationMathematical PhysicsLarge detector-systems performancePhysics010308 nuclear & particles physicsbusiness.industryDetectorResolution (electron density)LinearityInstrumentation and Detectors (physics.ins-det)Double-beta decay detectorsNuclear & Particles PhysicsOther Physical SciencesFull width at half maximumchemistryHigh pressurePhysical SciencesAnalysis and statistical methodsbusinessEnergy (signal processing)
researchProduct

The ATLAS Data Acquisition and High Level Trigger system

2016

Journal of Instrumentation 11(06), P06008 (2016). doi:10.1088/1748-0221/11/06/P06008

High level triggerComputer sciencedata acquisitionPhysics::Instrumentation and DetectorsLarge hadron collideronline filteringTrigger Concepts and Systems (Hardware and Software)Control and Monitor Systems Online01 natural sciencesOnline farms and online filteringData acquisitionRecopilación de datos[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental TechniquesInstrumentationMathematical PhysicsSettore FIS/01Online Farms and Online FilteringLarge Hadron ColliderControl and monitor systems onlineATLAS experimentATLASmedicine.anatomical_structureTrigger concepts and systems (hardware and software)Triggers and rulesComputer hardwareperformanceOnline farms andControl and monitor systems online; Data acquisition concepts; Online farms and online filtering; Trigger concepts and systems (hardware and software)Ciências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]Data Acquisition ConceptsATLAS detector; ATLAS experiment; CERN; Large Hadron ColliderATLAS experiment610Accelerator Physics and Instrumentation530LHC ATLAS High Energy Physics TriggerAtlas (anatomy)0103 physical sciencesmedicineddc:610ElectronicsInstrumentation (computer programming)Control and monitor systems online; Data acquisition concepts; Online farms and; online filtering; Trigger concepts and systems (hardware and software)010306 general physicsCiencias ExactasScience & Technology010308 nuclear & particles physicsbusiness.industryData acquisition conceptsFísicaAcceleratorfysik och instrumenteringtriggerSistema en líneaData flow diagrammonitoringHigh Energy Physics::Experimentbusiness
researchProduct

Development and Study of a Micromegas Pad-Detector for High Rate Applications

2015

In this paper, the design and the performance of two prototype detectors based on Micromegas technology with a pad readout geometry is discussed. In addition, two alternative implementations of a spark-resistent protection layer on top of the readout pads have been tested to optimize the charge-up behavior of the detector under high rates. The prototype detectors consist of 500 pads with a size of 5x4 mm, each connected to one independent readout channel, and cover an active area of 10x10 cm. The design of these prototypes and its associated readout infrastructure was developed in such a way that it can be easily adapted for large-size detector concepts.

High ratePhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and Detectorsbusiness.industryPhysics::Instrumentation and DetectorsDetectorFOS: Physical sciencesMicroMegas detectorInstrumentation and Detectors (physics.ins-det)Gaseous detectorsProtection layerDevelopment (differential geometry)Resistive couplingbusinessInstrumentationComputer hardwareCommunication channel
researchProduct

ATLAS TileCal Read Out Driver production

2007

The production tests of the 38 ATLAS TileCal Read Out Drivers (RODs) are presented in this paper. The hardware specifications and firmware functionality of the RODs modules, the test-bench and the test procedure to qualify the boards are described. Finally the performance results, the temperature studies and high rate tests are shown and discussed.

High ratebusiness.industryFirmwareTest proceduresComputer sciencecomputer.software_genrePerformance resultsmedicine.anatomical_structureAtlas (anatomy)medicineProduction (economics)businessInstrumentationcomputerMathematical PhysicsComputer hardwareComputingMethodologies_COMPUTERGRAPHICSJournal of Instrumentation
researchProduct

Coincidence of a high-fluence blazar outburst with a PeV-energy neutrino event

2016

The discovery of extraterrestrial very-high-energy neutrinos by the IceCube collaboration has launched a quest for the identification of their astrophysical sources. Gamma-ray blazars have been predicted to yield a cumulative neutrino signal exceeding the atmospheric background above energies of 100 TeV, assuming that both the neutrinos and the gamma-ray photons are produced by accelerated protons in relativistic jets. Since the background spectrum falls steeply with increasing energy, the individual events with the clearest signature of being of an extraterrestrial origin are those at PeV energies. Inside the large positional-uncertainty fields of the first two PeV neutrinos detected by Ic…

High-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaAstronomyNeutrino telescopeFOS: Physical sciencesGeneral Physics and AstronomyPhysics and Astronomy ; Neutrino ; Active Galactic NucleiAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesFluenceCoincidenceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrinoBlazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyActive Galactic NucleiHigh Energy Physics - PhenomenologyPhysics and AstronomyComputingMethodologies_DOCUMENTANDTEXTPROCESSINGNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)
researchProduct