Search results for "Lier"

showing 10 items of 906 documents

DARWIN: Towards the ultimate dark matter detector

2016

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the xenon will be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to WIMPs above a mass of 5 GeV/c2, such a detector with its large mass, low-energy …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsdouble beta decay7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNeutrino detectorHigh Energy Physics - Experiment (hep-ex)XenonWIMPPHOTOMULTIPLIERAXIONSphysics.ins-detsolar and atmospheric neutrinosPhysicsDark matter detectorTime projection chamberdark matter detectorsPhysicsSolar and atmospheric neutrinoInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsNeutrino detectorSOLAR NEUTRINOSGASPhysical SciencesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsGRAN SASSODark matter detectors; Double beta decay; Neutrino detectors; Solar and atmospheric neutrinosDark matterchemistry.chemical_elementFOS: Physical sciencesAstronomy & AstrophysicsLIQUID-XENON DETECTOR0202 Atomic Molecular Nuclear Particle And Plasma PhysicsSettore FIS/05 - Astronomia e AstrofisicaSEARCH0103 physical sciencesIsotopes of xenonZEPLIN-III[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)Science & Technology010308 nuclear & particles physicshep-exAstronomyAstronomy and Astrophysics0201 Astronomical And Space ScienceschemistryHigh Energy Physics::ExperimentSCINTILLATIONneutrino detectorsastro-ph.IMJournal of Cosmology and Astroparticle Physics
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JUNO sensitivity to low energy atmospheric neutrino spectra

2021

Atmospheric neutrinos are one of the most relevant natural neutrino sources that can be exploited to infer properties about cosmic rays and neutrino oscillations. The Jiangmen Underground Neutrino Observatory (JUNO) experiment, a 20 kton liquid scintillator detector with excellent energy resolution is currently under construction in China. JUNO will be able to detect several atmospheric neutrinos per day given the large volume. A study on the JUNO detection and reconstruction capabilities of atmospheric $\nu_e$ and $\nu_\mu$ fluxes is presented in this paper. In this study, a sample of atmospheric neutrino Monte Carlo events has been generated, starting from theoretical models, and then pro…

Physics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorsscintillation counter: liquidenergy resolutionAtmospheric neutrinoQC770-798Astrophysics7. Clean energy01 natural sciencesneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)particle source [neutrino]neutrinoneutrino: atmosphere[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Cherenkovneutrino/e: particle identificationenergy: low [neutrino]Jiangmen Underground Neutrino ObservatoryPhysicsJUNOphotomultiplierliquid [scintillation counter]primary [neutrino]neutrino: energy spectrumDetectoroscillation [neutrino]neutrinosMonte Carlo [numerical calculations]atmosphere [neutrino]QB460-466observatorycosmic radiationComputer Science::Mathematical Softwareproposed experimentNeutrinonumerical calculations: Monte CarloComputer Science::Machine LearningParticle physicsdata analysis methodAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayScintillatorComputer Science::Digital LibrariesNOStatistics::Machine LearningPE2_2neutrino: primaryneutrino: spectrumNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesddc:530structure010306 general physicsNeutrino oscillationEngineering (miscellaneous)Cherenkov radiationparticle identification [neutrino/mu]Scintillationneutrino/mu: particle identificationflavordetectorparticle identification [neutrino/e]010308 nuclear & particles physicsneutrino: energy: lowHigh Energy Physics::Phenomenologyspectrum [neutrino]resolutionenergy spectrum [neutrino]flux [neutrino]neutrino: particle source13. Climate actionHigh Energy Physics::Experimentneutrino: oscillationneutrino detector
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A Lagrangian framework for deriving triples and quadruples corrections to the CCSD energy.

2014

Using the coupled cluster Lagrangian technique, we have determined perturbative corrections to the coupled cluster singles and doubles (CCSD) energy that converge towards the coupled cluster singles, doubles, and triples (CCSDT) and coupled cluster singles, doubles, triples, and quadruples (CCSDTQ) energies, considering the CCSD state as the unperturbed reference state and the fluctua- tion potential as the perturbation. Since the Lagrangian technique is utilized, the energy corrections satisfy Wigner’s 2n + 1 rule for the cluster amplitudes and the 2n + 2 rule for the Lagrange multi- pliers. The energy corrections define the CCSD perturbation series, CCSD(T–n) and CCSD(TQ–n), which are ter…

Physics010304 chemical physicsGeneral Physics and AstronomyPerturbation (astronomy)010402 general chemistry01 natural sciences0104 chemical sciencessymbols.namesakeCoupled clusterAmplitudeQuantum mechanicsLagrange multiplier0103 physical sciencesPhysics::Atomic and Molecular ClusterssymbolsPerturbation theory (quantum mechanics)Physical and Theoretical ChemistryPhysics::Chemical PhysicsLagrangianThe Journal of chemical physics
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Total-variation methods for gravitational-wave denoising: Performance tests on Advanced LIGO data

2018

We assess total-variation methods to denoise gravitational-wave signals in real noise conditions, by injecting numerical-relativity waveforms from core-collapse supernovae and binary black hole mergers in data from the first observing run of Advanced LIGO. This work is an extension of our previous investigation where only Gaussian noise was used. Since the quality of the results depends on the regularization parameter of the model, we perform an heuristic search for the value that produces the best results. We discuss various approaches for the selection of this parameter, either based on the optimal, mean, or multiple values, and compare the results of the denoising upon these choices. Mor…

PhysicsArtificial neural network010308 nuclear & particles physicsGravitational waveNoise reductionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLIGOsymbols.namesakeAstrophysics - Solar and Stellar AstrophysicsBinary black holeGaussian noiseLagrange multiplier0103 physical sciencessymbolsWaveformAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)AlgorithmSolar and Stellar Astrophysics (astro-ph.SR)Physical Review D
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Perturbative triples corrections in state-specific multireference coupled cluster theory

2010

We formulated and implemented a perturbative triples correction for the state-specific multireference coupled cluster approach with singles and doubles suggested by Mukherjee and co-workers, Mk-MRCCSD [Mol. Phys. 94, 157 (1998)]. Our derivation of the energy correction [Mk-MRCCSD(T)] is based on a constrained search for stationary points of the Mk-MRCC energy functional together with a perturbative expansion with respect to the appearing triples cluster operator. The Lambda-Mk-MRCCSD(T) approach derived in this way consists in (1) a correction to the off-diagonal matrix elements of the effective Hamiltonian which is unique to coupled cluster methods based on the Jeziorski-Monkhorst ansatz, …

PhysicsDiagonalGeneral Physics and Astronomysymbols.namesakeCoupled clusterQuantum electrodynamicsLagrange multipliersymbolsPerturbation theory (quantum mechanics)Physical and Theoretical ChemistryHamiltonian (quantum mechanics)Wave functionMathematical physicsEnergy functionalAnsatzThe Journal of Chemical Physics
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Nonlinear nonviscous hydrodynamical models for charge transport in the framework of extended thermodynamic methods

2002

This paper develops a procedure, based on methods of extended thermodynamics, to design nonlinear hydrodynamical models for charge transport in metals or in semiconductors, neglecting viscous phenomena. Models obtained in this way allow the study of the motion of electric charges in the presence of arbitrary external electric fields and may be useful when one wishes to study phenomena in a neighborhood of a stationary nonequilibrium process: indeed, the drift velocity of the charge gas with respect to the crystal lattice is not regarded as a small parameter.

PhysicsDrift velocityStationary processNon-equilibrium thermodynamicsElectric chargeComputer Science ApplicationsNonlinear systemsymbols.namesakeClassical mechanicsModeling and SimulationElectric fieldLagrange multiplierModelling and SimulationsymbolsBalance equationMathematical and Computer Modelling
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A new radiation infrastructure for the Modular Earth Submodel System (MESSy, based on version 2.51)

2016

Abstract. The Modular Earth Submodel System (MESSy) provides an interface to couple submodels to a basemodel via a highly flexible data management facility (Jöckel et al., 2010). In the present paper we present the four new radiation related submodels RAD, AEROPT, CLOUDOPT and ORBIT. The submodel RAD (with shortwave radiation scheme RAD_FUBRAD) simulates the radiative transfer, the submodel AEROPT calculates the aerosol optical properties, the submodel CLOUDOPT calculates the cloud optical properties, and the submodel ORBIT is responsible for Earth orbit calculations. These submodels are coupled via the standard MESSy infrastructure and are largely based on the original radiation scheme of …

PhysicsECHAMEarth's orbit010504 meteorology & atmospheric sciencesMeteorologybusiness.industrylcsh:QE1-996.5Radiative forcingGeneral Medicine010501 environmental sciencesRadiative forcingModular design55101 natural scienceslcsh:Geologymodularised EMAC radiationErdsystem-ModellierungOrbit (dynamics)Radiative transferShortwave radiationAerospace engineeringbusinessStratosphere0105 earth and related environmental sciences
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PESIC: An Integrated Front-End for PET Applications

2007

An ASIC front-end has been developed for multi-anode photomultiplier based nuclear imaging devices. Its architecture has been designed to improve resolution and decrease pile-up probability in Positron Emission Tomography systems which employ continuous scintillator crystals. Analog computation elements are isolated from the photomultiplier by means of a current sensitive preamplifier stage. This allows digitally programmable adjustment of every anode gain, also providing better resolution in gamma event position calculation and a shorter front-end deadtime. The preamplifier stage also offers the possibility of using other types of photomultiplier devices such as SiPM. The ASIC architecture…

PhysicsFront and back endsPhotomultiplierSilicon photomultiplierPreamplifierAmplifierNuclear electronicsScintillation counterElectronic engineeringImage resolution2007 15th IEEE-NPSS Real-Time Conference
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Search for neutrino emission from gamma-ray sources with the Antares Telescope

2012

ANTARES is the first undersea neutrino detector ever built and presently the neutrino telescope with the largest effective area operating in the Northern Hemisphere. A three- dimensional array of photomultiplier tubes detects the Cherenkov light induced by the muons produced in the interaction of high energy neutrinos with the matter surrounding the detector. The detection of astronomical neutrino sources is one of the main goals of ANTARES. The search for point-like neutrino sources with the ANTARES telescope is described and the preliminary results obtained with data collected from 2007 to 2010 are shown. No cosmic neutrino source has been observed and neutrino flux upper limits have been…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhotomultiplierMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFOS: Physical sciencesCosmic raylaw.inventionTelescopeNeutrino detectorlawHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaCherenkov radiation
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Coordinate-free quantization of first-class constrained systems

1996

The coordinate-free formulation of canonical quantization, achieved by a flat-space Brownian motion regularization of phase-space path integrals, is extended to a special class of closed first-class constrained systems that is broad enough to include Yang-Mills type theories with an arbitrary compact gauge group. Central to this extension are the use of coherent state path integrals and of Lagrange multiplier integrations that engender projection operators onto the subspace of gauge invariant states.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsPure mathematicsQuantum PhysicsCanonical quantizationFOS: Physical sciencessymbols.namesakeHigh Energy Physics - Theory (hep-th)Gauge groupRegularization (physics)Lagrange multiplierPath integral formulationsymbolsCoherent statesQuantum Physics (quant-ph)Subspace topologyBrownian motion
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