Search results for "Instrumentation"

showing 10 items of 4914 documents

Detecting the Diffuse Supernova Neutrino Background with LENA

2014

Low energy neutrino astronomy (LENA) has been proposed as a next generation 50 kt liquid scintillator detector. Its large target mass allows us to search for the diffuse supernova neutrino background (DSNB), which was generated by the cumulative emissions of all core-collapse supernovae throughout the Universe. Indistinguishable background from reactor and atmospheric electron antineutrinos limits the detection window to the energy range between 9.5 MeV and 25 MeV. Depending on the mean supernova neutrino energy, about 5 to 10 events per year are expected in this energy window. The background from neutral current reactions of atmospheric neutrinos surpasses the DSNB by more than one order m…

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Solar neutrino problemNuclear physicsSupernovaAstrophysics - Solar and Stellar AstrophysicsNeutrino detectorMeasurements of neutrino speedNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for AstrophysicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)
researchProduct

Novel optical interferometry of synchrotron radiation for absolute electron beam energy measurements

2018

Abstract A novel interferometric method is presented for the measurement of the absolute energy of electron beams. In the year 2016, a pioneering experiment was performed using a 195 MeV beam of the Mainz Microtron (MAMI). The experimental setup consisted of two collinear magnetic undulators as sources of coherent optical synchrotron light and a high-resolving grating monochromator. Beam energy measurements required the variation of the relative undulator distance in the decimeter range and the analysis of the intensity oscillation length in the interference spectrum. A statistical precision of 1 keV was achieved in 1 h of data taking, while systematic uncertainties of 700 keV were present …

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsSpectrometer010308 nuclear & particles physicsbusiness.industrySynchrotron radiationFOS: Physical sciencesParticle acceleratorInstrumentation and Detectors (physics.ins-det)Undulator01 natural sciencesSynchrotronlaw.inventionOpticslaw0103 physical sciencesPhysics::Accelerator Physics010306 general physicsbusinessNuclear ExperimentInstrumentationMicrotronBeam (structure)Monochromator
researchProduct

Behavior of a trapezoid-based data acquisition system up to 100 kHz and beyond

2016

In this work, we investigated the ability of a high-purity germanium detector connected to a trapezoid-filter-based data acquisition system to reliably record signals in spite of high sample activities. By activating multiple Na$_{2}$CO$_{3}$ samples with different Na content, we were able to deduce efficiency, resolution and dead time of the system used as a function of the sample activity. Based on the results, we were able to find a setting which allows measurements of event rates up to 35~kHz per readout channel with an energy resolution of 0.3\% at the 2754 keV $^{24}$Na line.

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and Detectorsbusiness.industryResolution (electron density)FOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Dead timeSample (graphics)Semiconductor detectorData acquisitionOpticsLine (text file)Nuclear Experiment (nucl-ex)businessNuclear ExperimentInstrumentationEnergy (signal processing)Communication channel
researchProduct

Resonant detection and production of axions with atoms

2018

The axions and axion-like particles can be detected via a resonant atomic or molecular transition induced by axion absorption. The signal obtained in this process is second order in the axion-electron interaction constant and hence small. In this chapter, it is demonstrated that this signal may become first order in the axion-electron interaction constant if we allow the interference between the axion-induced transition amplitude and the transition amplitude induced by the electromagnetic radiation. Additionally, we show that the conventional scheme of producing axions from photons in a magnetic field may be improved if the field is replaced by an atomic medium in which photons scattering …

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsForward scatterHigh Energy Physics::PhenomenologyAstronomy and Astrophysics01 natural sciencesSignalAtomic and Molecular Physics and OpticsHigh Energy Physics::TheoryInterference (communication)0103 physical sciencesEffective lagrangianAtomic physics010306 general physicsAbsorption (electromagnetic radiation)AxionInternational Journal of Modern Physics A
researchProduct

Implementation of theP¯ANDA Planar-GEM tracking detector in Monte Carlo simulations

2018

Abstract The P ¯ ANDA experiment at FAIR will be performed to investigate different aspects of hadron physics using anti-proton beams interacting with a fixed nuclear target. The experimental setup consists of a complex series of detector components covering a large solid angle. A detector with a gaseous active media equipped with gas electron multiplier (GEM) technique will be employed to measure tracks of charged particles at forward direction in order to achieve a high momentum resolution. In this work, a full setup of the GEM tracking detector has been implemented in the P ¯ ANDA Monte Carlo simulation package (PandaRoot) based on the current technical and conceptual design, and the exp…

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsMonte Carlo methodDetectorSolid angleTracking (particle physics)01 natural sciencesRadiation lengthCharged particleComputational physicsPlanar0103 physical sciencesGas electron multiplier010306 general physicsInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
researchProduct

High Voltage Monolithic Active Pixel Sensors

2018

Ever higher demands on resolution and rate capability drive the development of particle tracking detectors. Especially at low momenta, multiple Coulomb scattering in the material of the detector is also strongly affecting the resolution of momentum measurements. While gas-based detectors such as drift chambers and time projection chambers can be built with very small amounts of material, their rate capability is limited by ageing and space charge effects. Hybrid semiconductor detectors on the other hand combine a depleted (silicon) sensor with a custom amplifier and readout chip. Pixelated devices especially can operate efficiently in very harsh rate and radiation environments such as the i…

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsbusiness.industryAmplifierDetectorHigh voltageSemiconductor deviceTracking (particle physics)Chip01 natural sciencesSpace charge030218 nuclear medicine & medical imagingSemiconductor detector03 medical and health sciences0302 clinical medicine0103 physical sciencesOptoelectronicsbusinessNuclear Physics News
researchProduct

A time-differential Mössbauer emission spectrometer with high efficiency and high time resolution

1986

A high-efficiency, high rate-capability, computer-based measuring setup for Time-Differential Mossbauer Spectroscopy was constructed. Applying NaI(Tl) and plastic scintillators for the detection of the 14.4 keV and 122 keV γ-radiation respectively, a superior timing (2, 3 ns FWHM) was achieved by a “fast-fast-ultra fast” timing method developed for that purpose.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAnalytical chemistryTime resolutionScintillatorCondensed Matter PhysicsAtomic and Molecular Physics and OpticsFull width at half maximumMössbauer spectroscopyPhysical and Theoretical ChemistryThin filmSpectroscopyDifferential (mathematics)Emission SpectrometerHyperfine Interactions
researchProduct

Results from the AMANDA telescope

2003

We present results from the AMANDA high energy neutrino telescope located at the South Pole. They include measurements of the atmospheric neutrino flux, search for UHE point sources, and diffuse sources producing electromagnetic/hadronic showers at the detector or close to it.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFluxCosmic rayAstrophysicsParticle detectorlaw.inventionMassless particleTelescopeNeutrino detectorlawHigh Energy Physics::ExperimentNeutrinoLeptonNuclear Physics A
researchProduct

Recent results from AMANDA II

2003

Abstract We present new data taken with the AMANDA-II neutrino telescope array. The AMANDA-II upgrade was completed at the beginning of 2000. It significantly extends the sensitivity of the 10-string AMANDA-B10 detector to high- and ultrahigh-energy neutrino fluxes into regions of interest for probing current astrophysical models which remain unexplored by other experiments.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeDetectorAstronomyCosmic rayAstrophysicsComputer Science::Computational GeometryAtomic and Molecular Physics and OpticsParticle detectorUpgradeNeutrino detectorHigh Energy Physics::ExperimentNeutrinoNuclear Physics B - Proceedings Supplements
researchProduct

Results from the AMANDA neutrino telescope

2004

The Amanda neutrino telescope at the South Pole has been taking data since 1996. Stepwise upgraded, it reached its final stage in January 2000. We present results from the search for extraterrestrial neutrinos, neutrinos from dark matter annihilation and magnetic monopoles.

PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyDark matterAstronomyAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSolar neutrino problemAtomic and Molecular Physics and Opticslaw.inventionTelescopeNeutrino detectorlawMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNuclear Physics B - Proceedings Supplements
researchProduct