Search results for "parametrization"

showing 10 items of 99 documents

Equivalent continuum-based upscaling of flow in discrete fracture networks: The fracture-and-pipe model

2021

Abstract. Predicting effective permeabilities of fractured rock masses is a key component of reservoir modelling. This is often realized with the discrete fracture network (DFN) method, where single-phase incompressible fluid flow is modelled in discrete representations of individual fractures in a network. Depending on the overall number of fractures, this can result in significant computational costs. Equivalent continuum models (ECM) provide an alternative approach by subdividing the fracture network into a grid of continuous medium cells, over which hydraulic properties are averaged for fluid flow simulations. While this has the advantage of lower computational costs and the possibility…

Physics::Fluid DynamicsPermeability (earth sciences)DiscretizationFlow (mathematics)Fracture (geology)Fluid dynamicsMechanicsAnisotropyParametrizationGeologyPhysics::GeophysicsPipe flow
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A new method for computing one-loop integrals

1994

We present a new program package for calculating one-loop Feynman integrals, based on a new method avoiding Feynman parametrization and the contraction due to Passarino and Veltman. The package is calculating one-, two- and three-point functions both algebraically and numerically to all tensor cases. This program is written as a package for Maple. An additional Mathematica version is planned later.

MapleFeynman parametrizationFeynman integralNumerical analysisElectroweak interactionFOS: Physical sciencesGeneral Physics and Astronomyengineering.materialNumerical integrationRenormalizationAlgebraHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Hardware and ArchitectureComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATIONComputer Science::Mathematical SoftwareengineeringContraction (operator theory)Mathematics
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Initial state in heavy ion collisions

2016

Abstract We briefly review advances in understanding the initial stages of a heavy ion collision. In particular the focus is on moving from parametrizing the initial state to calculating its properties from QCD, consistently with the description of hard probes and dilute-dense scattering experiments. Modeling the event-by-event fluctuating nuclear geometry in initial state calculations has significantly improved in recent years. We also discuss prospects of directly seeing effects of particle correlations created in the initial state in the experimental observables.

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsta114010308 nuclear & particles physicsScatteringheavy ion collisionsObservableCollision01 natural sciencesquark gluon plasmaquantum chromodynamics0103 physical sciencesQuark–gluon plasmaParticle010306 general physicsFocus (optics)ParametrizationNuclear and Particle Physics Proceedings
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Stopping powers of havar for 1.6, 2.3 and 3.2 MeV/u heavy ions

2000

Abstract Stopping powers of havar for 28,30 Si-, 36 Ar-, 54,56 Fe- and 80,84 Kr-ions with energies of 1.6, 2.3 and 3.2 MeV/u have been determined by a transmission technique. Sample foils are exposed to the direct beams. No previous data for havar with these ions have been published. The obtained results are brought together with literature havar data for 1 H-, 4 He-, 7 Li-, 11 B-, 12 C-, 14 N-, 16 O- and 127 I-ions at the same ion velocity. The experimental data are compared with the values predicted by the SRIM-2000 parametrization using Bragg’s rule. A systematic underestimation, by 6–23%, of the experimental stopping powers was observed. The empirical correction scheme of Thwaites has b…

Nuclear physicsNuclear and High Energy PhysicsChemistryEmpirical correctionStopping power (particle radiation)Atomic physicsInstrumentationParametrizationEffective nuclear chargeIonNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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2018

We show that the measured intrinsic octupole moments of $^{220}\mathrm{Rn}$, $^{224}\mathrm{Ra}$, and $^{226}\mathrm{Ra}$ constrain the intrinsic Schiff moments of $^{225}\mathrm{Ra}$, $^{221}\mathrm{Rn}$, $^{223}\mathrm{Rn}$, $^{223}\mathrm{Fr}$, $^{225}\mathrm{Ra}$, and $^{229}\mathrm{Pa}$. The result is a dramatically reduced uncertainty in intrinsic Schiff moments. Direct measurements of octupole moments in odd nuclei will reduce the uncertainty even more. The only significant source of nuclear-physics error in the laboratory Schiff moments will then be the intrinsic matrix elements of the time-reversal noninvariant interaction produced by $CP$-violating fundamental physics. Those matri…

Systematic errorPhysics010308 nuclear & particles physicsGeneral Physics and AstronomyActinide01 natural sciencesMatrix (mathematics)0103 physical sciencesFundamental physicsPhysics::Atomic PhysicsAtomic physics010306 general physicsParametrizationNuclear theoryPhysical Review Letters
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Toward Parametrization of Precipitating Shallow Cumulus Cloud Organization via Moisture Variance

2021

The influence of the initial vertical moisture profile on precipitating shallow cumulus cloud organization in terms of the column‐averaged moisture variance is investigated using large‐eddy simulations. Five idealized simulations based on the Rain in Cumulus over the Ocean field experiment with different initial moisture profiles are investigated. All cases simulate precipitating shallow cumulus convection in a marine sub‐tropical region under large‐scale subsidence. The results show that the moisture variance is mainly generated through the interaction of the moisture flux and the moisture gradient in the gradient production term at the top of the boundary layer. The development is charact…

Atmospheric ScienceMoisturePlanetary boundary layerCumulus cloudVariance (accounting)Atmospheric sciencesComputer Science::OtherPhysics::GeophysicsGeophysicsddc:551.5Space and Planetary ScienceComputer Science::Computational Engineering Finance and ScienceEarth and Planetary Sciences (miscellaneous)Environmental scienceParametrization (atmospheric modeling)Physics::Atmospheric and Oceanic PhysicsLarge eddy simulation
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2021

Abstract IceCube is a cubic-kilometer Cherenkov telescope operating at the South Pole. The main goal of IceCube is the detection of astrophysical neutrinos and the identification of their sources. High-energy muon neutrinos are observed via the secondary muons produced in charge current interactions with nuclei in the ice. Currently, the best performing muon track directional reconstruction is based on a maximum likelihood method using the arrival time distribution of Cherenkov photons registered by the experiment's photomultipliers. A known systematic shortcoming of the prevailing method is to assume a continuous energy loss along the muon track. However at energies >1 TeV the light yie…

PhysicsPhotomultiplierPhotonMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for Astrophysics7. Clean energy01 natural scienceslaw.inventionNuclear physicsTelescopelaw0103 physical sciencesHigh Energy Physics::ExperimentAngular resolutionNeutrino010306 general physics010303 astronomy & astrophysicsInstrumentationParametrizationMathematical PhysicsCherenkov radiationJournal of Instrumentation
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Neutrinoless double-beta decay and physics beyond the standard model

2012

Neutrinoless double beta decay is the most powerful tool to probe not only for Majorana neutrino masses but for lepton number violating physics in general. We discuss relations between lepton number violation, double beta decay and neutrino mass, review a general Lorentz invariant parametrization of the double beta decay rate, highlight a number of different new physics models showing how different mechanisms can trigger double beta decay, and finally discuss possibilities to discriminate and test these models and mechanisms in complementary experiments.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaLorentz covariance01 natural sciencesLepton numberHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Complementary experimentsDouble beta decay0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsParametrizationJournal of Physics G: Nuclear and Particle Physics
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Intercomparison of remote-sensing based evapotranspiration algorithms over amazonian forests

2019

Abstract Evapotranspiration (ET) is considered a key variable in the understanding of the Amazonian tropical forests and their response to climate change. Remote-Sensing (RS) based evapotranspiration models are presented as a feasible means in order to provide accurate spatially-distributed ET estimates over this region. In this work, the performance of four commonly used ET RS models was evaluated over Amazonia using Moderate Resolution Imaging Spectroradiometer (MODIS) data. RS models included i) Priestley-Taylor Jet Propulsion Laboratory (PT-JPL), ii) Penman-Monteith MODIS operative parametrization (PM-Mu), iii) Surface Energy Balance System (SEBS), and iv) Satellite Application Facility…

Global and Planetary ChangeAmazonian tropical forests; Terrestrial evapotranspiration; MODIS; Reanalysis010504 meteorology & atmospheric sciencesAmazonianCloud cover0211 other engineering and technologiesAmazonian tropical forestsClimate changeReanalysis02 engineering and technologyManagement Monitoring Policy and Law01 natural sciencesVariable (computer science)MODISEvapotranspirationEnvironmental scienceParametrization (atmospheric modeling)SatelliteModerate-resolution imaging spectroradiometerComputers in Earth SciencesTerrestrial evapotranspirationAlgorithm021101 geological & geomatics engineering0105 earth and related environmental sciencesEarth-Surface ProcessesInternational Journal of Applied Earth Observation and Geoinformation
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A simple equation for determining sea surface emissivity in the 3–15 µm region

2009

The high level of accuracy demanded for the sea surface temperature retrieval from infrared data requires an accurate determination of directional sea surface emissivity (SSE). Previous models have permitted calculating SSEs using a physical characterization of sea surface roughness and emission. However, these result in complex equations, and make an operational application difficult. This paper presents a simple SSE algorithm based on a parametrization of one of these models, which was selected as a reference since it reproduces SSE experimental data to a reasonable level of accuracy. The parametrization provides the SSE variation with observation angle and wind speed from a given nadir S…

Physics::Computational PhysicsPhysicsAATSRSurface finishWind speedComputer Science::PerformanceComputer Science::Mathematical SoftwareNadirEmissivitySurface roughnessGeneral Earth and Planetary SciencesRadiometryParametrizationRemote sensingInternational Journal of Remote Sensing
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