0000000001164810

AUTHOR

Franz Von Feilitzsch

showing 4 related works from this author

The next-generation liquid-scintillator neutrino observatory LENA

2012

We propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a next-generation neutrino observatory on the scale of 50 kt. The outstanding successes of the Borexino and KamLAND experiments demonstrate the large potential of liquid-scintillator detectors in low-energy neutrino physics. LENA's physics objectives comprise the observation of astrophysical and terrestrial neutrino sources as well as the investigation of neutrino oscillations. In the GeV energy range, the search for proton decay and long-baseline neutrino oscillation experiments complement the low-energy program. Based on the considerable expertise present in European and international research groups, the …

Neutrino detectors; Liquid-scintillator detectors; Low-energy neutrinos; Proton decay; Longbaseline neutrino beamsParticle physicsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaLongbaseline neutrino beamsFOS: Physical sciencesLow-energy neutrinos7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNONuclear physicsLiquid-scintillator detectorsHigh Energy Physics - Experiment (hep-ex)0103 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]Neutrino detectorsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsBorexinoPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Proton decaySolar neutrino problem[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for Astrophysics
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Fracture Processes Observed with A Cryogenic Detector

2006

In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time the energy release in fracture has been directly and accurately measured on a microscopic event-by-event basis. The energy threshold corresponds to the breaking of only a few hundred covalent bonds, a sensitivity some orders of magnitude greater than that of previou…

Physics - Instrumentation and Detectorsmedia_common.quotation_subjectDark matterGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciencesAsymmetryPower law010305 fluids & plasmasHigh Energy Physics - Experiment[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Time domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsmedia_commonPhysicsHurst exponent[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AutocorrelationAstrophysics (astro-ph)Instrumentation and Detectors (physics.ins-det)Computational physicsExponential functionOrders of magnitude (time)
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Fracture processes studied in CRESST

2005

In the early stages of running of the CRESST dark matter search with sapphire crystals as detectors, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time that the energy release in fracture has been accurately measured on a microscopic event-by-event basis. The energy distributions appear to follow a power law, dN/dE proportional to E-beta, similar to the Gutenberg-Richter power law for earthquake magnitudes, and after appropriat…

PhysicsNuclear and High Energy Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AutocorrelationDark matter01 natural sciencesPower law010305 fluids & plasmasComputational physicsNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]81.05.-t; 05.40; 07.90.+c; 29.40.-v0103 physical sciencesFracture (geology)Time domain[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationEvent (particle physics)Energy (signal processing)Noise (radio)
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Measurement of θ13 in Double Chooz using neutron captures on hydrogen with novel background rejection techniques

2016

The Double Chooz collaboration presents a measurement of the neutrino mixing angle θ[subscript 13] using reactor [bar over ν[subscript e]] observed via the inverse beta decay reaction in which the neutron is captured on hydrogen. This measurement is based on 462.72 live days data, approximately twice as much data as in the previous such analysis, collected with a detector positioned at an average distance of 1050 m from two reactor cores. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties. Accidental coincidences, the dominant background in this analysis, are suppressed by more than an order of magnitude with respec…

data analysis methodNuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsNeutrino Detectors and TelescopeGadoliniumnuclear reactor [antineutrino/e]energy spectrumchemistry.chemical_elementFluxmixing angle: measured [neutrino]CHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - Experimentflux [antineutrino]Flavor physicscapture [n]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interactionddc:530Neutron010306 general physicsPhysicsNeutrino Detectors and Telescopesbackground010308 nuclear & particles physicsoscillation [neutrino]suppressionDouble ChoozNeutron captureOscillationchemistryhydrogenInverse beta decayFlavor physicspectralHigh Energy Physics::ExperimentgadoliniumNeutrinoOrder of magnitudeexperimental results
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