0000000000205552

AUTHOR

Florian Kaether

showing 9 related works from this author

Journal of High Energy Physics

2014

The Double Chooz experiment presents improved measurements of the neutrino mixing angle $\theta_{13}$ using the data collected in 467.90 live days from a detector positioned at an average distance of 1050 m from two reactor cores at the Chooz nuclear power plant. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties with respect to previous publications, whereas the efficiency of the $\bar\nu_{e}$ signal has increased. The value of $\theta_{13}$ is measured to be $\sin^{2}2\theta_{13} = 0.090 ^{+0.032}_{-0.029}$ from a fit to the observed energy spectrum. Deviations from the reactor $\bar\nu_{e}$ prediction observed ab…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics - Instrumentation and DetectorsNeutrino Detectors and TelescopeFOS: Physical sciencesCHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)ExperimentDistortion0103 physical sciencesEnergy spectrum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsMixing (physics)PhysicsNeutrino Detectors and Telescopes010308 nuclear & particles physicsOscillationPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorFunction (mathematics)Instrumentation and Detectors (physics.ins-det)OscillationNeutrinoInstrumentation and Detectors
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Physics reach of the XENON1T dark matter experiment.

2016

The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section, based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds. The total electronic recoil background in $1$ tonne fiducial volume and ($1$, $12$) keV electronic recoil equivalent energy region, before applying any selection to discriminate between electronic and nuclear recoils, is $(1.80 \pm 0.15) \cdot 10^{-4}$ ($\rm{kg} \cdot day \cdot keV)^{-1}$, mainly due to the decay of $^{222}\rm{Rn}$ daughters inside the xenon target. The nu…

dark matter simulationsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsdark matter experimentFOS: Physical scienceschemistry.chemical_elementCosmic ray7. Clean energy01 natural sciencesdark matter simulationNuclear physicsRecoilXenonIonization0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysicsMuon010308 nuclear & particles physicsdark matter experimentsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)dark matter experiments; dark matter simulationschemistryNeutrinoNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Conceptual design and simulation of a water Cherenkov muon veto for the XENON1T experiment

2014

XENON is a direct detection dark matter project, consisting of a time projection chamber (TPC) that uses xenon in double phase as a sensitive detection medium. XENON100, located at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, is one of the most sensitive experiments of its field. During the operation of XENON100, the design and construction of the next generation detector (of ton-scale mass) of the XENON project, XENON1T, is taking place. XENON1T is being installed at LNGS as well. It has the goal to reduce the background by two orders of magnitude compared to XENON100, aiming at a sensitivity of $2 \cdot 10^{-47} \mathrm{cm}^{\mathrm{2}}$ for a WIMP mass of 50 GeV/c$^{2}$. With…

axionsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov and transition radiationCherenkov detectorPhysics::Instrumentation and DetectorsDark matterDetector modelling and simulations I (interaction of radiation with matterchemistry.chemical_elementFOS: Physical sciences01 natural scienceslaw.inventionNuclear physicsXenonWIMPlawCherenkov and transition radiation Detector modelling and simulations Cherenkov detectors Dark Matter detectorsetc.)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)Dark Matter detectors (WIMPsMathematical PhysicsCherenkov radiationetc)PhysicsMuonTime projection chamber010308 nuclear & particles physicsCherenkov detectorsDetectorAstrophysics::Instrumentation and Methods for Astrophysicsinteraction of photons with matterInstrumentation and Detectors (physics.ins-det)Cherenkov and transition radiation; Cherenkov detectors; Dark Matter detectors (WIMPs axions etc.); Detector modelling and simulations I (interaction of radiation with matter; interaction of hadrons with matter etc); interaction of photons with matter[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]interaction of hadrons with matterchemistryHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for AstrophysicsJOURNAL OF INSTRUMENTATION
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Precision Muon Reconstruction in Double Chooz

2014

We describe a muon track reconstruction algorithm for the reactor anti-neutrino experiment Double Chooz. The Double Chooz detector consists of two optically isolated volumes of liquid scintillator viewed by PMTs, and an Outer Veto above these made of crossed scintillator strips. Muons are reconstructed by their Outer Veto hit positions along with timing information from the other two detector volumes. All muons are fit under the hypothesis that they are through-going and ultrarelativistic. If the energy depositions suggest that the muon may have stopped, the reconstruction fits also for this hypothesis and chooses between the two via the relative goodness-of-fit. In the ideal case of a thro…

Nuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciencesSTRIPSDouble Chooz; Muon reconstruction; Neutrino detector[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]CHOOZScintillatorHigh Energy Physics - Experimentlaw.inventionNONuclear physicsNeutrino detectorHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]InstrumentationImage resolutionPhysicsMuonDetectorReconstruction algorithmInstrumentation and Detectors (physics.ins-det)Double ChoozNeutrino detectorPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentMuon reconstruction
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Muon capture on light isotopes measured with the Double Chooz detector

2016

Using the Double Chooz detector, designed to measure the neutrino mixing angle $\theta_{13}$, the products of $\mu^-$ capture on $^{12}$C, $^{13}$C, $^{14}$N and $^{16}$O have been measured. Over a period of 489.5 days, $2.3\times10^6$ stopping cosmic $\mu^-$ have been collected, of which $1.8\times10^5$ captured on carbon, nitrogen, or oxygen nuclei in the inner detector scintillator or acrylic vessels. The resulting isotopes were tagged using prompt neutron emission (when applicable), the subsequent beta decays, and, in some cases, $\beta$-delayed neutrons. The most precise measurement of the rate of $^{12}\mathrm C(\mu^-,\nu)^{12}\mathrm B$ to date is reported: $6.57^{+0.11}_{-0.21}\time…

PhysicsSemileptonic decayParticle physicseducation.field_of_studyMuon010308 nuclear & particles physicsPopulationneutrino physic01 natural sciencesMuon captureNuclear physics13. Climate action0103 physical sciencesHigh Energy Physics::ExperimentNeutronProduction (computer science)Neutrino010306 general physicsGround stateeducation
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The neutron background of the XENON100 dark matter search experiment

2013

TheXENON100 experiment, installed underground at the LaboratoriNazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering off xenon nuclei. This paper presents a study on the nuclear recoil background of the experiment, taking into account neutron backgrounds from (alpha, n) reactions and spontaneous fission due to natural radioactivity in the detector and shield materials, as well as muon-induced neutrons. Based on MonteCarlo simulations and using measured radioactive contaminations of all detector components, we predict the nuclear recoil backgrounds for the WIMP search results published by theXENO…

Nuclear and High Energy PhysicsParticle physicsLarge Underground Xenon experimentPhysics::Instrumentation and DetectorsDark matterGeant4Astrophysics::Cosmology and Extragalactic AstrophysicsWIMP Argon Programme01 natural sciencesNuclear physicsWIMPNuclear and High Energy Physics Neutron Background Dark Matter Search XENON TPC0103 physical sciencesNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSSpontaneous fissionPhysicsElastic scatteringFluxMuons010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsWeakly interacting massive particlesHigh Energy Physics::ExperimentSimulation
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Limits on spin-dependent WIMP-nucleon cross sections from 225 live days of XENON100 data

2013

We present new experimental constraints on the elastic, spin-dependent WIMP-nucleon cross section using recent data from the XENON100 experiment, operated in the Laboratori Nazionali del Gran Sasso in Italy. An analysis of 224.6 live days x 34 kg of exposure acquired during 2011 and 2012 revealed no excess signal due to axial-vector WIMP interactions with 129-Xe and 131-Xe nuclei. This leads to the most stringent upper limits on WIMP-neutron cross sections for WIMP masses above 6 GeV, with a minimum cross section of 3.5 x 10^{-40} cm^2 at a WIMP mass of 45 GeV, at 90% confidence level.

Cosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Dark matterGeneral Physics and AstronomyFOS: Physical sciences01 natural sciencesdark matterParticle detectorHigh Energy Physics - ExperimentNuclear physicsCross section (physics)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPseudovectorInstrumentation and Methods for Astrophysics (astro-ph.IM)Spin-½Physics010308 nuclear & particles physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Astrophysics - Instrumentation and Methods for AstrophysicsNucleonAstrophysics - Cosmology and Nongalactic Astrophysics
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Observation and applications of single-electron charge signals in the XENON100 experiment

2014

The XENON100 dark matter experiment uses liquid xenon in a time projection chamber (TPC) to measure xenon nuclear recoils resulting from the scattering of dark matter Weakly Interacting Massive Particles (WIMPs). In this paper, we report the observation of single-electron charge signals which are not related to WIMP interactions. These signals, which show the excellent sensitivity of the detector to small charge signals, are explained as being due to the photoionization of impurities in the liquid xenon and of the metal components inside the TPC. They are used as a unique calibration source to characterize the detector. We explain how we can infer crucial parameters for the XENON100 experim…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsDrift velocity[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsDark matterchemistry.chemical_elementFOS: Physical sciencesdouble phase TPC01 natural sciencesdark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonWIMPdouble phase TPC; photoionization; single electron; xenon0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsphotoionizationInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsTime projection chamber010308 nuclear & particles physicsScatteringDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)single electron3. Good health[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]xenonchemistryWeakly interacting massive particlesAtomic physicsAstrophysics - Instrumentation and Methods for AstrophysicsJ. Phys.
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Dark matter results from 225 live days of XENON100 data

2012

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3 \pm 0.6) \times 10^-3 events (kg day keVee)^-1 in the energy region of interest. A blind analysis of 224.6 live days \times 34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the pre-defined nuclear recoil energy range of 6.6-30.5 keVnr are consistent with the background expectation of (1.0 \pm 0.2) events. A Profile Likelihood analysis using a 6.6-43.3 keVnr energy range sets the most stringent limit o…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsLarge Underground Xenon experimentDark matterFOS: Physical sciencesGeneral Physics and AstronomyWIMP Argon Programme01 natural sciences7. Clean energyParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsLiquid XenonPhysicsRange (particle radiation)010308 nuclear & particles physicsDARK MATTERInstrumentation and Detectors (physics.ins-det)High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]DAMA/NaITPCPandaXDirect search for Dark MatterAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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