Search results for "Gamma"

showing 10 items of 3093 documents

"Table 6" of "First measurement of the quark to photon fragmentation function"

1995

3-JET events. Variable Z has been defined as E(gamma)/(E(gamma)+E(had)), where E(gamma) is the energy of the hard photon in 'photon-jet', E(had) is the energy of the rest hadrons in jet. Ycut is jet resolution parameter (see paper).

FDSIG/SIGE+ E- --> 3JETAstrophysics::High Energy Astrophysical PhenomenaE+ E- ScatteringIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentE+ E- --> GAMMA QUARK QUARKBAR90.912Jet ProductionCross SectionE+ E- --> (HADRONS) 2HADRON
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"Table 7" of "First measurement of the quark to photon fragmentation function"

1995

3-JET events. Variable Z has been defined as E(gamma)/(E(gamma)+E(had)), where E(gamma) is the energy of the hard photon in 'photon-jet', E(had) is the energy of the rest hadrons in jet. Ycut is jet resolution parameter (see paper).

FDSIG/SIGE+ E- --> 3JETAstrophysics::High Energy Astrophysical PhenomenaE+ E- ScatteringIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentE+ E- --> GAMMA QUARK QUARKBAR90.912Jet ProductionCross SectionE+ E- --> (HADRONS) 2HADRON
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Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

2014

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV - PeV range at the level of $10^{-8}\, \mathrm{GeV}\, \mathrm{cm}^{-2}\, \mathrm{s}^{-1}\, \mathrm{sr}^{-1}$ per flavor and reject a purely atmospheric explanation for the combined 3-year data at $5.7 \sigma$. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotrop…

FLUXACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)TELESCOPESolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyASTRONOMYAstronomySolar neutrino problemBLAZARSPhysics and AstronomyNeutrino detector13. Climate actionLEPTONSJETSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyEMISSIONAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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"Table 3" of "Measurement of the eta and eta' transition form factors at q**2 = 112-GeV**2."

2006

Transition form factors at Q**2 = 112 GeV**2.

FORM-FACTORElectron productionE+ E- ScatteringE+ E- --> ETAPRIME GAMMAExclusiveE+ E- --> ETA GAMMA10.58
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KFAS : Exponential Family State Space Models in R

2017

State space modelling is an efficient and flexible method for statistical inference of a broad class of time series and other data. This paper describes an R package KFAS for state space modelling with the observations from an exponential family, namely Gaussian, Poisson, binomial, negative binomial and gamma distributions. After introducing the basic theory behind Gaussian and non-Gaussian state space models, an illustrative example of Poisson time series forecasting is provided. Finally, a comparison to alternative R packages suitable for non-Gaussian time series modelling is presented.

FOS: Computer and information sciencesStatistics and ProbabilityaikasarjatGaussianNegative binomial distributionforecastingPoisson distribution01 natural sciencesStatistics - ComputationMethodology (stat.ME)010104 statistics & probability03 medical and health sciencessymbols.namesake0302 clinical medicineExponential familyexponential familyGamma distributionStatistical inferenceState spaceApplied mathematicsSannolikhetsteori och statistik030212 general & internal medicine0101 mathematicsProbability Theory and Statisticslcsh:Statisticslcsh:HA1-4737Computation (stat.CO)Statistics - MethodologyMathematicsR; exponential family; state space models; time series; forecasting; dynamic linear modelsta112state space modelsSeries (mathematics)RStatistics; Computer softwaresymbolsStatistics Probability and Uncertaintytime seriesSoftwaredynamic linear models
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Strongly interacting Fermi gases with density imbalance

2005

We consider density-imbalanced Fermi gases of atoms in the strongly interacting, i.e. unitarity, regime. The Bogoliubov-deGennes equations for a trapped superfluid are solved. They take into account the finite size of the system, as well as give rise to both phase separation and FFLO type oscillations in the order parameter. We show how radio-frequency spectroscopy reflects the phase separation, and can provide direct evidence of the FFLO-type oscillations via observing the nodes of the order parameter.

FOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesElectromagnetic radiation010305 fluids & plasmasSuperconductivity (cond-mat.supr-con)SuperfluidityCondensed Matter - Strongly Correlated ElectronsCondensed Matter::Superconductivity0103 physical sciences010306 general physicsSpectroscopyPhysicsCondensed Matter::Quantum GasesStrongly Correlated Electrons (cond-mat.str-el)UnitarityCondensed matter physicsCondensed Matter::OtherCondensed Matter - SuperconductivityFermionCondensed Matter - Other Condensed MatterQuantum electrodynamicsFermi gasOther Condensed Matter (cond-mat.other)Dimensionless quantityFermi Gamma-ray Space Telescope
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Pairing gap and in-gap excitations in trapped fermionic superfluids

2004

We consider trapped atomic Fermi gases with Feshbach-resonance enhanced interactions in pseudogap and superfluid temperatures. We calculate the spectrum of RF(or laser)-excitations for transitions that transfer atoms out of the superfluid state. The spectrum displays the pairing gap and also the contribution of unpaired atoms, i.e. in-gap excitations. The results support the conclusion that a superfluid, where pairing is a many-body effect, was observed in recent experiments on RF spectroscopy of the pairing gap.

FOS: Physical sciencesRoton01 natural sciences010305 fluids & plasmasSuperfluiditySuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsSuperfluid state0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Physics::Atomic Physics010306 general physicsFeshbach resonanceSpectroscopyCondensed Matter - Statistical MechanicsPhysicsCondensed Matter::Quantum GasesQuantum PhysicsMultidisciplinaryCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsStatistical Mechanics (cond-mat.stat-mech)Strongly Correlated Electrons (cond-mat.str-el)Condensed Matter::OtherCondensed Matter - SuperconductivityPairingPseudogapQuantum Physics (quant-ph)Fermi Gamma-ray Space Telescope
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Effect of Salt-Loading and Spontaneous Hypertension on in Vitro Metabolism of [1-14C]Linoleic and [2-14C]Dihomo-γ-linolenic Acids

1993

The present study compared the effect of spontaneous hypertension and salt-loading on in vitro metabolism of 18:2n-6 (linoleic acid) and 20:3n-6 (dihomo-gamma-linolenic acid). Ten weanling spontaneously hypertensive rats (SHR) and 10 normotensive Wistar-Kyoto rats (WKY) maintained on a rodent lab chow were given tap water with (n = 5) or without (n = 5) addition of 1% NaCl for 4 weeks. Thereafter, animals were killed and liver microsomes were prepared. Aliquots of microsomes suspended in the phosphate-sucrose buffer containing MgCl2, ATP, CoA, and NADPH were incubated with 0.3 microCi of [1-14C]-18:2n-6 or [2-14C]-20:3n-6 at 37 degrees C for 15 min. The activity of delta 6- and delta 5-desa…

Fatty Acid DesaturasesMalemedicine.medical_specialtyLinolenic AcidsEndocrinology Diabetes and MetabolismLinoleic acidPhospholipidProstaglandinIn Vitro TechniquesSodium ChlorideRats Inbred WKYBiochemistryLinoleic Acidchemistry.chemical_compoundRats Inbred SHRInternal medicinemedicineAnimalsgamma-Linolenic Acidgamma-Linolenic acidchemistry.chemical_classificationMetabolismRatsEndocrinologyLinoleic AcidschemistryBiochemistryHypertensionMicrosomes LiverMicrosomeArachidonic acidPolyunsaturated fatty acidBiochemical Medicine and Metabolic Biology
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Caratterizzazione ESR di composti fenolici: nuovi materiali per la dosimetria in campo misto neutroni-gamma

2014

Fenoli Dosimetria ESR Campo misto neutroni gamma GadolinioSettore FIS/01 - Fisica SperimentaleSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)
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Dikerogammarus villosus (Crustacea : Amphipoda): another invasive species in Lake Geneva

2004

According to field observations performed in 2002 and 2003, the amphipod species Dikerogammarus villosus (Sowinsky, 1894) is now well established in Lake Geneva. The author predicts that this and future invasions by D. villosus will have serious effects on freshwater ecosystems.

Fishery[SDV.EE] Life Sciences [q-bio]/Ecology environmentAmphipodaEcologyDikerogammarus villosusBiologybiology.organism_classificationFreshwater ecosystemCrustaceanEcology Evolution Behavior and SystematicsInvasive speciesComputingMilieux_MISCELLANEOUS[ SDV.EE ] Life Sciences [q-bio]/Ecology environment
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