Search results for "53"

showing 10 items of 2908 documents

Observation of e + e − → ηψ(2S) at center-of-mass energies from 4.236 to 4.600 GeV

2021

Journal of high energy physics 2021(10), 177 (2021). doi:10.1007/JHEP10(2021)177

ExoticsNuclear and High Energy Physicsmeasured [channel cross section]e+-e− ExperimentsQuarkoniumannihilation [electron positron]QC770-798electron positron: annihilationetaParticle and resonance productionMeasure (mathematics)530Standard deviationNONuclear physicsSubatomär fysikCross section (physics)e+-e��� Experimentsenergy dependence: measured [cross section]Astronomi astrofysik och kosmologiNuclear and particle physics. Atomic energy. RadioactivitySubatomic PhysicsAstronomy Astrophysics and Cosmologyddc:530e+-e− Experiments Exotics Particle and resonance production Quarkoniumpsi(3685)PhysicsBESe(+)-e(-) ExperimentsDetectorstatistical [error]electron positron --> eta psi(3685)e +-e − Experimentselectron positron: colliding beamsBeijing Stor4.236-4.600 GeV-cmsCollisionerror: statisticalYield (chemistry)e-e Experimentselectron positron --> eta psi(3685)colliding beams [electron positron]High Energy Physics::ExperimentCenter of masscross section: energy dependence: measuredchannel cross section: measuredStorage ringexperimental results
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Search for new phenomena in final states with large jet multiplicities and missing transverse momentum at s√=8 TeV proton-proton collisions using the…

2013

A search is presented for new particles decaying to large numbers (7 or more) of jets, with missing transverse momentum and no isolated electrons or muons. This analysis uses 20.3 fb[superscript −1] of pp collision data at s√ = 8 TeV collected by the ATLAS experiment at the Large Hadron Collider. The sensitivity of the search is enhanced by considering the number of b-tagged jets and the scalar sum of masses of large-radius jets in an event. No evidence is found for physics beyond the Standard Model. The results are interpreted in the context of various simplified supersymmetry-inspired models where gluinos are pair produced, as well as an mSUGRA/CMSSM model.

ExoticsPhysics::Instrumentation and DetectorsCiencias FísicasPhysics beyond the Standard ModelElectron01 natural sciences7. Clean energyHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)Jets[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QChadron-hadron scatteringPhysicsGluinoLarge Hadron ColliderSettore FIS/01 - Fisica SperimentaleATLAS experimentSupersymmetryATLASJet physicsPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCParticle Physics - ExperimentCIENCIAS NATURALES Y EXACTASNuclear and High Energy PhysicsParticle physicsHadron-Hadron Scattering; Jet physics; Supersymmetry ExoticsCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]Scalar (mathematics)FOS: Physical sciencesHadron-hadron scattering530Nuclear physics0103 physical sciencesFysikddc:530High Energy Physics010306 general physicsScience & TechnologyMuon010308 nuclear & particles physicssupersymmetry; hadron-hadron scattering; jet physics; exoticsHigh Energy Physics::PhenomenologyexoticsFísica//purl.org/becyt/ford/1.3 [https]Hadron scatteringAstronomíaHADRON-HADRON COLLISIONSExperimental High Energy PhysicsHigh Energy Physics::ExperimentSupersymmetrysupersymmetry
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Rentabilidad de una pequeña explotación agraria en Vall de Uxó, 1721-1739

1982

Una serie de circunstancias nos ha permitido conocer la contabilidad de una pequeña explotación en la llanura costera valenciana, en Vall de Uxó, límite sur de la actual provincia de Castellón. En un proceso típico los arrendatarios de los derechos señoriales del Ducado de Villahermosa no pueden hacer frente a sus pagos y sus tierras son confiscadas; la cosecha está por recoger y se conceden temporalmente en administración a un campesino del lugar. Al no surgir postores en las subastas que se realizan, parte de las tierras siguen en manos de este labrador, a quien un buen día se le exigen cuentas de su administración. La relación pormenorizada de los gastos que ha realizado en el cultivo de…

Explotaciones agrariasDP1-402Modern history 1453-Rendimientos económicosD204-475Siglo XVIIIReligious studiesHistory of SpainVall de UxóRevista de Historia Moderna
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Numerical stochastic perturbation theory in the Schrödinger functional

2013

The Schr\"odinger functional (SF) is a powerful and widely used tool for the treatment of a variety of problems in renormalization and related areas. Albeit offering many conceptual advantages, one major downside of the SF scheme is the fact that perturbative calculations quickly become cumbersome with the inclusion of higher orders in the gauge coupling and hence the use of an automated perturbation theory framework is desirable. We present the implementation of the SF in numerical stochastic perturbation theory (NSPT) and compare first results for the running coupling at two loops in pure SU(3) Yang-Mills theory with the literature.

FIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIHigh Energy Physics - Latticeddc:530Lattice QCDPerturbation theoryStochastic quantizationLangevin equations
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

2016

We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles ra…

FLUORESCENCE YIELDAstronomymagnetic monopolemagnetic fieldAstrophysics7. Clean energy01 natural sciencesObservatoryUHE Cosmic Raysair-showerMonte Carlo010303 astronomy & astrophysicsMagnetic Monopolesmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicscritical phenomenaFLUORESCENCE YIELD; ENERGY LOSS; DETECTORAugerMagnetic fieldobservatoryLorentz factorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical Phenomenaspatial distribution [showers]LorentzENERGY LOSSatmosphere [showers]energyFLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]airmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Magnetic monopoleFOS: Physical sciencesCosmic rayNuclear physicssymbols.namesakecosmic rays0103 physical sciencesddc:530High Energy PhysicsDETECTORCiencias Exactasfluorescence [detector]Pierre Auger Observatorybackground010308 nuclear & particles physicsFísicaASTROFÍSICAUniversefluxultrarelativistic magnetic monopolesAir shower13. Climate actionExperimental High Energy PhysicsrelativisticgalaxyENERGY-LOSS
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IceTop : the surface component of IceCube

2012

IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an air shower array with an area of 1 km2. The detector allows a detailed exploration of the mass composition of primary cosmic rays in the energy range from about 100 TeV to 1 EeV by exploiting the correlation between the shower energy measured in IceTop and the energy deposited by muons in the deep ice. In this paper we report on the technical design, construction and installation, the trigger and data acquisition systems as well as the software framework for calibration, reconstruction and simulation. Finally the first experience from commissioning and operating the detector and the performance as an …

FLUXNuclear and High Energy PhysicsAir showerPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAir shower; Cosmic rays; Detector; IceCube; IceTopFOS: Physical sciencesCosmic rayddc:500.27. Clean energy01 natural sciencesIceCube Neutrino ObservatoryIceCubeShowerData acquisitioncosmic raysDIGITIZATION0103 physical sciencesSHOWERSCalibrationddc:530Instrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationCosmic raysRemote sensingPhysicsMuondetector010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyDetectorENERGY-SPECTRUMAir showerPhysics and AstronomySIMULATIONIceTopHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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Search for relativistic magnetic monopoles with IceCube

2012

We present the first results in the search for relativistic magnetic monopoles with the IceCube detector, a subsurface neutrino telescope located in the South Polar ice cap containing a volume of 1 km$^{3}$. This analysis searches data taken on the partially completed detector during 2007 when roughly 0.2 km$^{3}$ of ice was instrumented. The lack of candidate events leads to an upper limit on the flux of relativistic magnetic monopoles of $\Phi_{\mathrm{90%C.L.}}\sim 3\e{-18}\fluxunits$ for $\beta\geq0.8$. This is a factor of 4 improvement over the previous best experimental flux limits up to a Lorentz boost $\gamma$ below $10^{7}$. This result is then interpreted for a wide range of mass …

FLUXSELECTIONAMANDANuclear and High Energy PhysicsParticle physicsProton decayCherenkov detectorPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleFOS: Physical sciencesddc:500.201 natural scienceslaw.inventionIceCube Neutrino ObservatoryPhysics::GeophysicsIceCubelaw0103 physical sciencesGrand Unified Theoryddc:530NEUTRINO TELESCOPE010306 general physicsCherenkov radiationPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsFIELDS85-05Physics and AstronomyNeutrino detectorAstrophysics - High Energy Astrophysical Phenomena
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Probing the origin of cosmic-rays with extremely high energy neutrinos using the IceCube Observatory

2013

We have searched for extremely high energy neutrinos using data taken with the IceCube detector between May 2010 and May 2012. Two neutrino induced particle shower events with energies around 1 PeV were observed, as reported previously. In this work, we investigate whether these events could originate from cosmogenic neutrinos produced in the interactions of ultra-high energy cosmic-rays with ambient photons while propagating through intergalactic space. Exploiting IceCube's large exposure for extremely high energy neutrinos and the lack of observed events above 100 PeV, we can rule out the corresponding models at more than 90% confidence level. The model independent quasi-differential 90% …

FLUXSELECTIONFERMI-LATNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLIMIT01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Particle showerObservatory0103 physical sciencesddc:530010306 general physicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMRange (particle radiation)COSMOGENIC NEUTRINOS010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyPERFORMANCECOMPONENTMODELPhysics and Astronomy13. Climate actionIntergalactic travelHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSYSTEMAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Search for sterile neutrino mixing using three years of IceCube DeepCore data

2017

Physical review / D 95(11), 112002(2017). doi:10.1103/PhysRevD.95.112002

FLUXSterile neutrinoParticle physicsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciences530High Energy Physics - ExperimentOSCILLATION EXPERIMENTSHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesTRACK RECONSTRUCTIONddc:530010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomySolar neutrino problemLINE-EXPERIMENT-SIMULATORMODELHigh Energy Physics - PhenomenologyNeutrino detectorPhysics and AstronomyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrino
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Safety assurance of an industrial robotic control system using hardware/software co-verification

2022

As a general trend in industrial robotics, an increasing number of safety functions are being developed or re-engineered to be handled in software rather than by physical hardware such as safety relays or interlock circuits. This trend reinforces the importance of supplementing traditional, input-based testing and quality procedures which are widely used in industry today, with formal verification and model-checking methods. To this end, this paper focuses on a representative safety-critical system in an ABB industrial paint robot, namely the High-Voltage electrostatic Control system (HVC). The practical convergence of the high-voltage produced by the HVC, essential for safe operation, is f…

FOS: Computer and information sciencesFormal Languages and Automata Theory (cs.FL)Formal methodsVerificationComputer Science - Formal Languages and Automata Theory:Teknisk kybernetikk: 553 [VDP]VDP::Teknisk kybernetikk: 553RoboticsComputer Science - RoboticsVDP::Technical cybernetics: 553:Technical cybernetics: 553 [VDP]VerifikasjonFormelle metoderRobotikkRobotics (cs.RO)Software
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