Search results for "F0"

showing 10 items of 98 documents

Highly sensitive monoclonal antibody-based immunoassays for boscalid analysis in strawberries

2018

Boscalid is an agrochemical recently developed for crop protection and the most significant member of the succinate dehydrogenase inhibitor group of fungicides. In this study, a collection of high-affinity monoclonal antibodies was generated to boscalid. By using a series of haptens with a linker at alternative tethering sites of the boscalid framework, specific antibodies were isolated as well as antibodies that also recognized the main boscalid metabolite. Two immunoassays were developed using different ELISA formats. Optimized assays displayed very high sensitivities (limits of detection were near 0.01 µg/L). Trueness and precision for the determination of the target analyte in strawberr…

NiacinamideAnalyteStrawberriesmedicine.drug_classFungicideMetaboliteEnzyme-Linked Immunosorbent AssayQuechersMonoclonal antibodyFragaria01 natural sciencesAnalytical Chemistrychemistry.chemical_compoundLimit of DetectionmedicineDetection limitResidue (complex analysis)Chromatographymedicine.diagnostic_test010405 organic chemistryChemistryBiphenyl Compounds010401 analytical chemistryAntibodies MonoclonalGeneral MedicineCompetitive ELISAFungicides Industrial0104 chemical sciencesMetabolite M510F01FruitImmunoassayMonoclonal antibodiesBoscalidHaptensHaptenFood ScienceFood Chemistry
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Unitarized Chiral Perturbation Theory in a finite volume: scalar meson sector

2011

We develop a scheme for the extraction of the properties of the scalar mesons f0(600), f0(980), and a0(980) from lattice QCD data. This scheme is based on a two-channel chiral unitary approach with fully relativistic propagators in a finite volume. In order to discuss the feasibility of finding the mass and width of the scalar resonances, we analyze synthetic lattice data with a fixed error assigned, and show that the framework can be indeed used for an accurate determination of resonance pole positions in the multi-channel scattering.

Nuclear and High Energy PhysicsChiral perturbation theoryeffect [threshold]MesonNuclear TheoryHigh Energy Physics::LatticeFOS: Physical scienceschiral [perturbation theory]f0(980)a0(980)Nuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeLattice (order)relativistic [propagator]unitarityddc:530energy levelsScalar mesonnumerical calculationsMathematical physicsPhysicsFinite volume methodScatteringscalar [resonance]High Energy Physics - Lattice (hep-lat)PropagatorFísicascalar mesonLattice QCDf0(600)boundary conditionpole [resonance]High Energy Physics - Phenomenologyfinite size
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Study of the f(2)(1270) , f(2)'(1525) , f(0)(1370) and f(0)(1710) in the J/psi radiative decays

2009

In this paper we present an approach to study the radiative decay modes of the J/psi into a photon and one of the tensor mesons f (2)(1270) , f' (2)(1525) , as well as the scalar ones f (0)(1370) and f (0)(1710) . Especially, we compare predictions that emerge from a scheme where the states appear dynamically in the solution of vector meson-vector meson scattering amplitudes to those from a (admittedly naive) quark model. We provide evidence that it might be possible to distinguish amongst the two scenarios, once improved data are available.

Nuclear and High Energy PhysicsParticle physicsPhotonMesonScalar (mathematics)Radiative decayhadronic decay [J/psi(3100)]01 natural sciencesf0(1710)bound state [vector meson]radiative decay [J/psi(3100)]0103 physical sciencesRadiative transferddc:530f0(1370)Tensor010306 general physicsnumerical calculationsdecay modes [J/psi(3100)]Physicsquark modelf2(1525)ratio [width]010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyQuark modelFísicascalar meson3. Good healthScattering amplitudef2(1270)tensor mesonHigh Energy Physics - Phenomenologywidth [J/psi(3100)]High Energy Physics::Experiment
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Apport de matières organiques exogènes en agriculture: indicateur de potentialité de stockage de carbone dans les sols et définition de classes de di…

2007

CT3; absent

P33 - Chimie et physique du solCarboneAzote[SDV]Life Sciences [q-bio]Stockagehttp://aims.fao.org/aos/agrovoc/c_5192Fertilisationhttp://aims.fao.org/aos/agrovoc/c_5268http://aims.fao.org/aos/agrovoc/c_7427Matière organiquehttp://aims.fao.org/aos/agrovoc/c_2810AGRONOMIEEngraishttp://aims.fao.org/aos/agrovoc/c_1301disponibilité d'élément nutritifhttp://aims.fao.org/aos/agrovoc/c_5387http://aims.fao.org/aos/agrovoc/c_10795DéchetSolSTOCKAGE DE CARBONE[ SDV ] Life Sciences [q-bio]P35 - Fertilité du solhttp://aims.fao.org/aos/agrovoc/c_2867CompostBASE DE DONNEESLisierClassificationFumierPHYSIQUE[SDV] Life Sciences [q-bio]http://aims.fao.org/aos/agrovoc/c_8307http://aims.fao.org/aos/agrovoc/c_1795http://aims.fao.org/aos/agrovoc/c_1653CHIMIE ORGANIQUEhttp://aims.fao.org/aos/agrovoc/c_7156http://aims.fao.org/aos/agrovoc/c_16602F04 - Fertilisation
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Adapter localement les prévisions climatiques saisonnières : désagrégation stochastique et interpolation spatiale.

2013

6 pages; International audience; Un panorama est fait des méthodes de descente d’échelles permettant de passer de prévisions climatiques saisonnières de large-échelle à des séries locales journalières. L’exemple des générateurs stochastiques de temps est appliqué à la prévision des récoltes de sorgho au Kenya, dans le cadre du programme ANR PICREVAT. Une méthode d’interpolation spatiale des paramètres des générateurs est testée, pour obtenir des séries journalières de précipitations en tout point du territoire. Les séries générées sont utilisées en entrée du modèle agronomique SARRA-H.

P40 - Météorologie et climatologieF01 - Culture des plantesU10 - Informatique mathématiques et statistiques[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry[SDU.STU.GC] Sciences of the Universe [physics]/Earth Sciences/Geochemistrydésagrégationgénérateur stochastiqueprécipitationsrendementsprévision saisonnière[ SDU.STU.GC ] Sciences of the Universe [physics]/Earth Sciences/Geochemistry
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Climatic gradients along the windward slopes of Mount Kenya and their implication for crop risks. Part 2 : crop sensitivity.

2016

16 pages; International audience; Mount Kenya is an equatorial mountain whose climatic setting is fairly simple (two rainy seasons in March–May, the Long Rains, and October–December, the Short Rains) though concealing significant spatial variations related to elevation and aspect (part I, Camberlin et al., 2014). This part II is dedicated to the sensitivity of sorghum yields to climate variability in space and time, with a focus on the intra-seasonal characteristics of the rainy seasons. To that aim we use the crop model SARRA-H calibrated for the region and fed with rainfall, temperature, wind speed, humidity and solar radiation data over the period 1973–2001 at three stations located on t…

P40 - Météorologie et climatologie[SDV.SA.AGRO]Life Sciences [q-bio]/Agricultural sciences/AgronomySARRA-Hintra-seasonal componentsrainy seasonhttp://aims.fao.org/aos/agrovoc/c_9000024http://aims.fao.org/aos/agrovoc/c_10176[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/Climatology[ SDV.SA.AGRO ] Life Sciences [q-bio]/Agricultural sciences/AgronomyF01 - Culture des planteshttp://aims.fao.org/aos/agrovoc/c_7244ComputingMilieux_MISCELLANEOUSPrécipitationhttp://aims.fao.org/aos/agrovoc/c_24894rainfall variabilityU10 - Informatique mathématiques et statistiquesModélisation des culturescrop modelKenyaVariation saisonnièreRendement des cultureselevation gradientshttp://aims.fao.org/aos/agrovoc/c_4086[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatologyhttp://aims.fao.org/aos/agrovoc/c_6161sorghum[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/Climatology
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"Decay Phase-Space Volume of Partial Waves" of "Light isovector resonances in $\pi^- p \to \pi^-\pi^-\pi^+ p$ at 190 GeV/${\it c}$"

2018

Decay phase-space volume $I_{aa}$ for the 14 selected partial waves as a function of $m_{3\pi}$, normalized such that $I_{aa}(m_{3\pi} = 2.5~\text{GeV}/c^2) = 1$. The wave index $a$ represents the quantum numbers that uniquely define the partial wave. The quantum numbers are given by the shorthand notation $J^{PC} M^\varepsilon [$isobar$] \pi L$. We use this notation to label the decay phase-space volume in the column headers. The labels are identical to the ones used in the column headers of the table of the transition amplitudes. $I_{aa}$ is calculated using Monte Carlo integration techniques for fixed $m_{3\pi}$ values, which are given in the first column, in the range from 0.5 to 2.5 Ge…

PI- P --> PI2(2005)- PLight-Meson SpectroscopyIsobar ModelPI- P --> PI- F2(1270) PAmplitude AnalysisPI- P --> PI1(1600)- PDiffractivePI- P --> A1(1420)- PPI- P --> A1(1260)- PPI- P --> A2(1320)- PPI- P --> A1(1640)- PPI- P --> A4(2040)- PPI- P --> PI- RHO0 PPI- P --> PI- F0(980) PPI- P --> PI- PI- PI+ PPI- P --> PI2(1670)- PPI- P --> A2(1700)- PExclusivePI- P --> PI(1800)- PPI- P --> PI2(1880)- PPion-Proton Scattering
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"Transition Amplitudes" of "Light isovector resonances in $\pi^- p \to \pi^-\pi^-\pi^+ p$ at 190 GeV/${\it c}$"

2018

Real and imaginary parts of the normalized transition amplitudes $\mathcal{T}_a$ of the 14 selected partial waves in the 1100 $(m_{3\pi}, t')$ cells (see Eq. (12) in the paper). The wave index $a$ represents the quantum numbers that uniquely define the partial wave. The quantum numbers are given by the shorthand notation $J^{PC} M^\varepsilon [$isobar$] \pi L$. We use this notation to label the transition amplitudes in the column headers. The $m_{3\pi}$ values that are given in the first column correspond to the bin centers. Each of the 100 $m_{3\pi}$ bins is 20 MeV/$c^2$ wide. Since the 11 $t'$ bins are non-equidistant, the lower and upper bounds of each $t'$ bin are given in the column he…

PI- P --> PI2(2005)- PLight-Meson SpectroscopyIsobar ModelPI- P --> PI- F2(1270) PAmplitude AnalysisPI- P --> PI1(1600)- PDiffractivePartial-Wave AmplitudePI- P --> A1(1420)- PPI- P --> A1(1260)- PPI- P --> A2(1320)- PPI- P --> A1(1640)- PPI- P --> A4(2040)- PPI- P --> PI- RHO0 PPI- P --> PI- F0(980) PPI- P --> PI- PI- PI+ PPI- P --> PI2(1670)- PPI- P --> A2(1700)- PExclusive19.0PI- P --> PI(1800)- PPI- P --> PI2(1880)- PPion-Proton ScatteringAMP
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Algebraic Quantization, Good Operators and Fractional Quantum Numbers

1995

The problems arising when quantizing systems with periodic boundary conditions are analysed, in an algebraic (group-) quantization scheme, and the ``failure" of the Ehrenfest theorem is clarified in terms of the already defined notion of {\it good} (and {\it bad}) operators. The analysis of ``constrained" Heisenberg-Weyl groups according to this quantization scheme reveals the possibility for new quantum (fractional) numbers extending those allowed for Chern classes in traditional Geometric Quantization. This study is illustrated with the examples of the free particle on the circumference and the charged particle in a homogeneous magnetic field on the torus, both examples featuring ``anomal…

PhysicsGeometric quantizationHigh Energy Physics - TheoryFree particleQuantization (signal processing)FOS: Physical sciencesStatistical and Nonlinear PhysicsMatemática Aplicada81S1081R99Ehrenfest theoremQuantum number58F06High Energy Physics - Theory (hep-th)Fractional quantum Hall effectCuantización algebraicaCuántica de números fraccionadosAlgebraic numberQuantumMathematical PhysicsMathematical physics
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Relative velocities for radial motion in expanding Robertson-Walker spacetimes

2011

The expansion of space, and other geometric properties of cosmological models, can be studied using geometrically defined notions of relative velocity. In this paper, we consider test particles undergoing radial motion relative to comoving (geodesic) observers in Robertson-Walker cosmologies, whose scale factors are increasing functions of cosmological time. Analytical and numerical comparisons of the Fermi, kinematic, astrometric, and the spectroscopic relative velocities of test particles are given under general circumstances. Examples include recessional comoving test particles in the de Sitter universe, the radiation-dominated universe, and the matter-dominated universe. Three distinct …

PhysicsSuperluminal motionPhysics and Astronomy (miscellaneous)SpacetimeGeodesicmedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)83F05 83C99General Relativity and Quantum CosmologyUniverseMetric expansion of spaceGeneral Relativity and Quantum CosmologyClassical mechanicsDe Sitter universeFermi coordinatesTest particleMathematical Physicsmedia_commonGeneral Relativity and Gravitation
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