0000000000205592

AUTHOR

Christian Buck

showing 4 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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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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Status of Light Sterile Neutrino Searches

2020

A number of anomalous results in short-baseline oscillation may hint at the existence of one or more light sterile neutrino states in the eV mass range and have triggered a wave of new experimental efforts to search for a definite signature of oscillations between active and sterile neutrino states. The present paper aims to provide a comprehensive review on the status of light sterile neutrino searches in mid-2019: we discuss not only the basic experimental approaches and sensitivities of reactor, source, atmospheric, and accelerator neutrino oscillation experiments but also the complementary bounds arising from direct neutrino mass experiments and cosmological observations. Moreover, we r…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBibliographyddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsOscillationHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Cosmological modelHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentAtmospheric neutrinoNeutrinoAstrophysics - Cosmology and Nongalactic Astrophysics
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