Search results for "methods"

showing 10 items of 4526 documents

Laboratory astrophysics survey of key x-ray diagnostic lines using a microcalorimeter on an electron beam ion trap

2000

Cosmic plasma conditions created in an electron beam ion trap (EBIT) make it possible to simulate the dependencies of key diagnostic X-ray lines on density, temperature, and excitation conditions that exist in astrophysical sources. We used a microcalorimeter for such laboratory astrophysics studies because it has a resolving power ≈1000, quantum efficiency approaching 100%, and a bandwidth that spans the X-ray energies from 0.2 keV to 10 keV. Our microcalorimeter, coupled with an X-ray optic to increase the effective solid angle, provides a significant new capability for laboratory astrophysics measurements. Broadband spectra obtained from the National Institute of Standards and Technology…

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementFizikai tudományokAstrophysicsSpectral lineNeonTermészettudományokAtomic processeIonizationPhysics::Atomic PhysicsAtomic dataNuclear and High Energy PhysicPhysicsArgonKryptonAstronomy and AstrophysicsLine: IdentificationPlasmaX-rays: GeneralchemistrySpace and Planetary ScienceAstrophysical plasmaMethods: Laboratory plasmaAtomic physicsElectron beam ion trap
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CALOS: an experiment to study the solar corona with an array of NTD Ge microcalorimeters

2002

In response to the Italian Space Agency announcement "New Ideas for Space Missions", we have proposed an observatory "CALorimetri per Osservazioni Solari" (CALOS) that will perform spatially resolved (Deltatheta similar to 2) X-ray spectroscopy of the solar corona over the 0.1 - 10 keV band using an array of NTD germanium microcalorimeters. The observatory will also include an X-ray polarimeter of radically new design that will study the hard X-ray solar emission and its polarization and will serve as a flare alarm.

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenachemistry.chemical_elementSolar coronaGermaniummicrocalorimeterAstrophysicsSpace explorationlaw.inventionX-raySettore FIS/05 - Astronomia E AstrofisicaOpticslawObservatoryAstrophysics::Solar and Stellar AstrophysicsSpectroscopyPhysicsX-ray astronomybusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyPolarimeterPolarization (waves)chemistryPhysics::Space PhysicsbusinessFlareAIP Conference Proceedings
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Deep sea tests of a prototype of the KM3NeT digital optical module

2014

The first prototype of a photo-detection unit of the future KM3NeT neutrino telescope has been deployed in the deepwaters of the Mediterranean Sea. This digital optical module has a novel design with a very large photocathode area segmented by the use of 31 three inch photomultiplier tubes. It has been integrated in the ANTARES detector for in-situ testing and validation. This paper reports on the first months of data taking and rate measurements. The analysis results highlight the capabilities of the new module design in terms of background suppression and signal recognition. The directionality of the optical module enables the recognition of multiple Cherenkov photons from the same (40)Kd…

Physics::Instrumentation and DetectorsAstrophysics::Instrumentation and Methods for AstrophysicsFísica
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Calibration strategy of the JUNO experiment

2021

We present the calibration strategy for the 20 kton liquid scintillator central detector of the Jiangmen Underground Neutrino Observatory (JUNO). By utilizing a comprehensive multiple-source and multiple-positional calibration program, in combination with a novel dual calorimetry technique exploiting two independent photosensors and readout systems, we demonstrate that the JUNO central detector can achieve a better than 1% energy linearity and a 3% effective energy resolution, required by the neutrino mass ordering determination. peerReviewed

Physics::Instrumentation and DetectorsAstrophysics::Instrumentation and Methods for AstrophysicsneutriinotHigh Energy Physics::Experimentfysiikkakalibrointi
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A method for detection of muon induced electromagnetic showers with the ANTARES detector

2012

The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved.

Physics::Instrumentation and DetectorsAtmospheric muonsDecay productsNeutrino telescopeElectromagnetic shower identification01 natural sciences7. Clean energyneutrino telescope electromagnetic shower identification high energy muons energy reconstruction; high energy muons; neutrino telescope; electromagnetic shower identification; energy reconstructionMuon neutrinoNEUTRINO TELESCOPE010303 astronomy & astrophysicsInstrumentationEnergy reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsHigh energy muonNeutrino detectorMuon colliderNeutrino astronomyFísica nuclearNeutrinoNeutrino telescope; Energy reconstruction; High energy muonsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUXNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Charged current[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayMuon neutrinoNuclear physicsElectromagnetism0103 physical sciencesHigh energy physicsneutrino telescope electromagnetic shower identification high energy muons energy reconstructionInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARES010308 nuclear & particles physicsCharged particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADATEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrino telescopesElectro-magnetic showersHigh energy muons
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Fabry-Pérot Interferometer : construction, calibration and developement

2015

The work presented in this thesis concentrates on the construction and development of a Fabry-Perot Interferometer (FPI). Resonance ionization spectroscopy (RIS) is a powerful technique for the extraction of nuclear structure, namely nuclear spins, moments and changes in mean-square charge radii. However, due to the pulsed nature of the laser, the technique may be limited by the laser linewidth to low resolution spectroscopy. This thesis presents the construction and characterization of a Fabry-Perot Interferometer in order to measure the laser linewidth and to calibrate the wavelength of a pulsed Ti:Sapphire laser in "Narrowband" mode (<1 GHz). The FPI has been directly utilized in the mea…

Physics::Instrumentation and DetectorsFabry-PerotspektroskopiaAstrophysics::Instrumentation and Methods for AstrophysicsPhysics::OpticsPhysics::Atomic PhysicsIGISOL
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"Table 1" of "A low-mass dark matter search using ionization signals in XENON100"

2018

WIMP exclusion limit on the spin-independent WIMP-nucleon scattering cross section at 90% confidence level.

Physics::Instrumentation and DetectorsNuclear TheoryAstrophysics::Instrumentation and Methods for AstrophysicsHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsSIGWIMP NUCLEON --&gt; X
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Performance study of the fast timing Cherenkov detector based on a microchannel plate PMT

2017

Prototype of the fast timing Cherenkov detector, applicable in high-energy collider experiments, has been developed basing on the modified Planacon XP85012 MCP-PMT and fused silica radiators. We present the reasons and description of the MCP-PMT modification, timing and amplitude characteristics of the prototype including the summary of the detector's response on particle hits at oblique angles and MCP-PMT performance at high illumination rates. peerReviewed

Physics::Instrumentation and DetectorsQuantitative Biology::Tissues and OrgansCherenkov detectorsAstrophysics::Instrumentation and Methods for Astrophysics
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902]

Physics::Instrumentation and DetectorsSolar neutrinoAstrophysicsUPPER LIMITPHOTON FRACTION01 natural sciences7. Clean energyneutrinoObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pionAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCOSMIC-RAYScosmic ray detectorsand other elementary particle detectorsCosmic neutrino backgroundNEUTRINOSFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFLUXFERMI-LATNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTORCosmic RayPionmuon0103 physical sciencesNeutrino010306 general physicsCosmic raysPierre Auger ObservatoryMuon010308 nuclear & particles physicsFísicaand other elementary particlesUltra-high energy cosmic raysPERFORMANCECosmic rayneutrino flavor; air showers; surface detector; observatory; atmosphere; Auger; cosmic radiation; energy spectrum13. Climate actionHigh Energy Physics::Experiment
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Neutrino oscillation studies with IceCube-DeepCore

2016

IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make…

Physics::Instrumentation and DetectorsSolar neutrinopoleinteraction [neutrino nucleon]PINGU01 natural sciences7. Clean energyneutrino nucleon: interactionIceCubeenergy: thresholdAstronomi astrofysik och kosmologineutrino: atmosphereAstronomy Astrophysics and Cosmologydetector [neutrino]Physicsneutrino: energy spectrumoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicsatmosphere [neutrino]threshold [energy]mass difference [neutrino]Cosmic neutrino backgroundneutrino: detectorNeutrino detectorPhysique des particules élémentairesMeasurements of neutrino speedNeutrinoperformanceNuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceddc:500.2530neutrino: energySOUTH-POLE0103 physical sciencesddc:530010306 general physicsNeutrino oscillation010308 nuclear & particles physicsICEenergy spectrum [neutrino]Solar neutrino problemneutrino: mixing anglePhysics and Astronomyenergy [neutrino]High Energy Physics::Experimentneutrino: oscillationNeutrino astronomyMATTERSYSTEMmixing angle [neutrino]experimental results
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