Search results for "Particle physics"

showing 10 items of 6826 documents

Mass dependence of inclusive nuclear $\phi$ photoproduction

2003

Based on a prior determination of the $\phi$ selfenergy in a nuclear medium we perform a theoretical study of inclusive $\phi$ photoproduction in nuclei, looking at the $A$ dependence of the cross sections for different $\phi$ momenta. We find sizeable reductions in the nuclear cross sections with respect to the elementary one, using a $\phi$ selfenergy which implies a width about six times the free one at normal nuclear density. The calculations are done to match the set up for an ongoing experiment at {\it SPring8/Osaka} which should provide valuable information on the renormalization of the $\phi$ properties in nuclei.

RenormalizationPhysicsNuclear physicsNuclear and High Energy PhysicsParticle physicsNuclear TheoryNuclear TheoryFísicaNuclear ExperimentNuclear theoryNuclear density
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Complex mass renormalization in EFT

2010

We consider an effective field theory of unstable particles (resonances) using the complex-mass renormalization. As an application we calculate the masses and the widths of the $\rho$ meson and the Roper resonance.

RenormalizationPhysicsParticle physicsRoper resonanceHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MesonHigh Energy Physics::LatticeNuclear TheoryEffective field theoryFOS: Physical sciencesNuclear Experiment
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Radiative Improvement of the Lattice Nonrelativistic QCD Action Using the Background Field Method and Application to the Hyperfine Splitting of Quark…

2011

We present the first application of the background field method to nonrelativistic QCD (NRQCD) on the lattice in order to determine the one-loop radiative corrections to the coefficients of the NRQCD action in a manifestly gauge-covariant manner. The coefficients of the $\mathbit{\ensuremath{\sigma}}\ifmmode\cdot\else\textperiodcentered\fi{}\mathbit{B}$ term in the NRQCD action and the four-fermion spin-spin interaction are computed at the one-loop level; the resulting shift of the hyperfine splitting of bottomonium is found to bring the lattice predictions in line with experiment.

RenormalizationPhysicsQuantum chromodynamicsParticle physicsBackground field methodHigh Energy Physics::LatticeLattice (order)Quantum electrodynamicsRadiative transferGeneral Physics and AstronomyQuarkoniumEffective actionHyperfine structurePhysical Review Letters
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Response of GAFChromic® HD-V2 film dosimeter in 10-300 Gy dose range for radiation testing of electronic devices

2019

The study reported in this paper aimed to investigate the response of a GAFChromic? HD-V2 film dosimeter in the dose range between 10 and 300 Gy, normally used to perform irradiation tests on electronic devices with a 60Co gamma-ray irradiator. The well-defined linearity of response in terms of absorbance as a function of absorbed dose, easiness of handling and data analysis of irradiated dosimeters, reproducibility, stability, and insensitivity to visible light and most of the environmental parameters, make HD-V2 film a flexible, inexpensive and reliable dose measurement device. The study has shown a fogging effect of the dosimeter response since its value changes over time. Strategies and…

ReproducibilityRange (particle radiation)HD-V2 filmDosimeterMaterials scienceGafchromic dosimetryRadiation testingElectronic deviceNuclear Energy and EngineeringDoseGamma-ray irradiationAbsorbed doseCalibrationlcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityIrradiationElectronicsSafety Risk Reliability and QualityBiomedical engineeringNuclear Technology and Radiation Protection
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Time-dependent resonance interaction energy between two entangled atoms under nonequilibrium conditions

2018

We consider the time-dependent resonance interaction energy between two identical atoms, one in the ground state and the other in an excited state, and interacting with the vacuum electromagnetic field, during a nonequilibrium situation such as the dynamical atomic self-dressing process. We suppose the two atoms prepared in a correlated, symmetric or antisymmetric, state. Since the atoms start from a nonequilibrium conditions, their interaction energy is time dependent. We obtain, at second order in the atom-field coupling, an analytic expression for the time-dependent resonance interaction energy between the atoms. We show that this interaction vanishes when the two atoms are outside the l…

Resonance interaction Casimir-Polder effect non equilibrium systems.High Energy Physics - TheoryCondensed Matter::Quantum GasesElectromagnetic fieldPhysicsQuantum PhysicsField (physics)Antisymmetric relationFOS: Physical sciencesNon-equilibrium thermodynamicsInteraction energy01 natural sciencesResonance (particle physics)010305 fluids & plasmasHigh Energy Physics - Theory (hep-th)Excited state0103 physical sciencesPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsAtomic physicsQuantum Physics (quant-ph)010306 general physicsGround statePhysical Review A
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A New Method of Velocity Estimation Based on Variable Temporal Basis Using Incremental Encoder

1997

Abstract This paper deals with analysis and synthesis of algorithms for digital conditioning of signals generated by incremental encoders to estimate velocity of rotating devices for control purposes. Main objectives are to obtain high accuracy at low and high velocity and low tracking delays during accelerations. A digital conditioning method is described, Which uses a polynomial of order n whose coefficients are updated so as to fit the n+1 most recent velocity data acquired on a variable temporal basis. Digital sinlulations and experimental findings are shown with the ainl to validate the proposed estimation method and compare it with other methods.

Rotary encoderPolynomialBasis (linear algebra)Control theoryVelocity estimationHigh velocityTracking (particle physics)EncoderVariable (mathematics)MathematicsIFAC Proceedings Volumes
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Search for ultrahigh-energy tau neutrinos with IceCube

2012

The first dedicated search for ultrahigh-energy (UHE) tau neutrinos of astrophysical origin was performed using the IceCube detector in its 22-string configuration with an instrumented volume of roughly 0.25  km3. The search also had sensitivity to UHE electron and muon neutrinos. After application of all selection criteria to approximately 200 live-days of data, we expect a background of 0.60±0.19(stat)+0.56−0.58(syst) events and observe three events, which after inspection, emerge as being compatible with background but are kept in the final sample. Therefore, we set an upper limit on neutrinos of all flavors from UHE astrophysical sources at 90% C.L. of E2νΦ90(νx)<16.3×10−8  GeV cm−2…

SELECTIONAMANDANuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaINDUCED CASCADESCosmic rayddc:500.2PROPAGATIONAstrophysicsElectron01 natural sciencesAmanda0103 physical sciencesEARTHddc:530Ultrahigh energy010306 general physicsPropagationSelectionPhysicsRange (particle radiation)Muon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsEarthPhysics and AstronomyInduced CascadesTELESCOPESHigh Energy Physics::ExperimentNeutrinoTelescopes
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Search for neutrino-induced particle showers with IceCube-40

2013

We report on the search for neutrino-induced particle-showers, so-called cascades, in the IceCube-40 detector. The data for this search was collected between April 2008 and May 2009 when the first 40 IceCube strings were deployed and operational. Three complementary searches were performed, each optimized for different energy regimes. The analysis with the lowest energy threshold (2 TeV) targeted atmospheric neutrinos. A total of 67 events were found, consistent with the expectation of 41 atmospheric muons and 30 atmospheric neutrino events. The two other analyses targeted a harder, astrophysical neutrino flux. The analysis with an intermediate threshold of 25 TeV lead to the observation of…

SELECTIONAMANDANuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayCASCADESSCATTERINGddc:530High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMMuonICEHigh Energy Physics::PhenomenologySolar neutrino problemMODELPhysics and AstronomyNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)SYSTEM
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First Observation of PeV-Energy Neutrinos with IceCube

2013

We report on the observation of two neutrino-induced events which have an estimated deposited energy in the IceCube detector of 1.04 $\pm$ 0.16 and 1.14 $\pm$ 0.17 PeV, respectively, the highest neutrino energies observed so far. These events are consistent with fully contained particle showers induced by neutral-current $\nu_{e,\mu,\tau}$ ($\bar\nu_{e,\mu,\tau}$) or charged-current $\nu_{e}$ ($\bar\nu_{e}$) interactions within the IceCube detector. The events were discovered in a search for ultra-high energy neutrinos using data corresponding to 615.9 days effective livetime. The expected number of atmospheric background is $0.082 \pm 0.004 \text{(stat)}^{+0.041}_{-0.057} \text{(syst)}$. T…

SELECTIONParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)ATMOSPHERIC MUONAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayddc:500.201 natural sciencesCHARMIceCube Neutrino Observatory0103 physical sciencesddc:550SCATTERING010303 astronomy & astrophysicsCharged currentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMNeutral current010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyICEGlashow resonancePERFORMANCE3. Good healthPhysics and AstronomyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSYSTEMAstrophysics - Cosmology and Nongalactic AstrophysicsBar (unit)
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An Information Aggregation and Analytics System for ATLAS Frontier

2019

International audience; ATLAS event processing requires access to centralized database systems where information about calibrations, detector status and data-taking conditions are stored. This processing is done on more than 150 computing sites on a world-wide computing grid which are able to access the database using the Squid-Frontier system. Some processing workflows have been found which overload the Frontier system due to the Conditions data model currently in use, specifically because some of the Conditions data requests have been found to have a low caching efficiency. The underlying cause is that non-identical requests as far as the caching are actually retrieving a much smaller num…

SQLQC1-999Complex event processingcomputer.software_genre01 natural sciencesprogrammingdata compilation0103 physical sciencesSpark (mathematics)[INFO]Computer Science [cs]010306 general physicsactivity reportcomputer.programming_languageDatabase010308 nuclear & particles physicsbusiness.industryPhysicsATLASCentralized databaseData modelAnalyticsefficiencyContainer (abstract data type)interfacedata managementUser interfacebusinesscomputerParticle Physics - Experimentperformance
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