0000000000241665

AUTHOR

H. H. J. Ten Kate

showing 5 related works from this author

Conceptual design of the International Axion Observatory (IAXO)

2014

The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal-to-noise ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, currently the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$ and thus probing a large fraction of the currently unexplored axion and ALP parameter space. IAXO will also be sensitive to solar axions produced by mechanisms mediated by the axion-electron coupling $g_{…

MICROPICPhysics - Instrumentation and DetectorsPhotonaxionsParameter space7. Clean energyHigh Energy Physics - ExperimentDark Matter detectors (WIMPs axions etc.)High Energy Physics - Experiment (hep-ex)Observatoryetc.)Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc)Detectors and Experimental TechniquesInstrumentationMathematical PhysicsPhysicsGEMsolar [axion]Dark Matter Detectors (Wimps Axions etc.)MicroMegas detectorX-ray detectorsInstrumentation and Detectors (physics.ins-det)Dark Matter detectors (WIMPs axions etc.); Large detector systems for particle and astroparticle physics; Micropattern gaseous detectors (MSGC GEM THGEM RETHGEM MHSP MICROPIC MICROMEGAS InGrid etc); X-ray detectors; Instrumentation; Mathematical PhysicssolarobservatoryMICROMEGASMHSPaxion-like particlesproposed experimentaxions ; dark matter detectors ; x-ray detectors ; Micropattern gaseous detectors ; large detector systems for particle and astroparticle physicsMicromegasX-ray detectorParticle physicsoptics [X-ray]FOS: Physical sciencesSuperconducting magnetMicropattern gaseous detectors (MSGCddc:610Axionactivity reportDark Matter detectors (WIMPssuperconductivity [magnet]etc)HelioscopeLarge detector systems for particle and astroparticle physicssensitivityInGridRETHGEMOrders of magnitude (time)axionLarge detector systems for particle and astroparticle physicTHGEMMicropattern Gaseous Detectors (MSGC Gem THGEM Rethgem MHSP Micropic Micromegas In Grid; etc)
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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
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The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)

2015

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 13th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2013; Asilomar Conference Grounds Monterey Peninsula; United States; 8 September 2013 through 13 September 2013. The International Axion Observatory (IAXO) is a proposed 4th-generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 - 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling gaγ down to a few ×10-12 GeV-1 for a wide range of axion masses up to ∼ 0.25 eV. This is an improvement over the currently best …

QCD axionParticle physicsPhysics::Instrumentation and DetectorsDark matterPhysics and Astronomy(all)01 natural sciences7. Clean energymagnetic helioscopeHigh Energy Physics::TheoryQCD axionsAstroparticle PhysicsAxionObservatory0103 physical sciencesDark matterQCD axions; magnetic helioscope; dark matterDark Matterddc:530Detectors and Experimental Techniques010306 general physicsAxionAstroparticle physicsPhysicsHelioscope010308 nuclear & particles physicsAxion Dark Matter ExperimentHigh Energy Physics::PhenomenologyStrong CP problemIAXOStrong CP ProblemALPStrong CP problemAstroparticle physicsCERN Axion Solar TelescopeParticle Physics - ExperimentHelioscopesPhysics Procedia
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Future axion searches with the International Axion Observatory (IAXO)

2013

Çetin, Serkant Ali (Dogus Author) -- Conference full title: 6th Symposium on Large TPCs for Low Energy Rare Event Detection; Paris; France; 17 December 2012 through 19 December 2012. The International Axion Observatory (IAXO) is a new generation axion helioscope aiming at a sensitivity to the axion-photon coupling of gaγ ∼ few × 10-12 GeV-1, i.e. 1-1.5 orders of magnitude beyond the one achieved by CAST, currently the most sensitive axion helioscope. The main elements of IAXO are an increased magnetic field volume together with extensive use of x-ray focusing optics and low background detectors, innovations already successfully tested in CAST. Additional physics cases of IAXO could include …

PhysicsHistoryParticle physicssolar axionOrders of Magnitude010308 nuclear & particles physicsRare event detectionSingle photon detectorsLow Background Detectors01 natural sciencesdark matterWhite DwarfsComputer Science ApplicationsEducationLow energyObservatory0103 physical sciencessolar axions; dark matter; Single photon detectorssolar axionsddc:530X-ray Focusing Optics010306 general physicsAxion
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Baby MIND: a magnetized segmented neutrino detector for the WAGASCI experiment

2017

T2K (Tokai-to-Kamioka) is a long-baseline neutrino experiment in Japan designed to study various parameters of neutrino oscillations. A near detector complex (ND280) is located 280~m downstream of the production target and measures neutrino beam parameters before any oscillations occur. ND280's measurements are used to predict the number and spectra of neutrinos in the Super-Kamiokande detector at the distance of 295~km. The difference in the target material between the far (water) and near (scintillator, hydrocarbon) detectors leads to the main non-cancelling systematic uncertainty for the oscillation analysis. In order to reduce this uncertainty a new WAter-Grid-And-SCintillator detector …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciencesCosmic rayScintillator01 natural sciences7. Clean energy030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineSilicon photomultiplierOptics0103 physical sciencesDetectors and Experimental TechniquesNeutrino oscillationphysics.ins-detInstrumentationMathematical PhysicsPhysicsMuon010308 nuclear & particles physicsbusiness.industryDetectorInstrumentation and Detectors (physics.ins-det)Neutrino detectorHigh Energy Physics::ExperimentLarge scale cryogenic liquid detectors [8]NeutrinobusinessJournal of Instrumentation
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