Search results for " high energy physics"

showing 10 items of 8412 documents

Chiral symmetry andπ-πscattering in the covariant spectator theory

2014

The π-π scattering amplitude calculated with a model for the quark-antiquark interaction in the framework of the Covariant Spectator Theory (CST) is shown to satisfy the Adler zero constraint imposed by chiral symmetry. The CST formalism is established in Minkowski space and our calculations are performed in momentum space. We prove that the axial-vector Ward-Takahashi identity is satisfied by our model. Then we show that, similarly to what happens within the Bethe-Salpeter formalism, application of the axial-vector Ward Takahashi identity to the CST π-π scattering amplitude allows us to sum the intermediate quark-quark interactions to all orders. Thus, the Adler self-consistency zero for π…

Ward–Takahashi identityPhysicsNuclear and High Energy PhysicsChiral symmetryBethe–Salpeter equation010308 nuclear & particles physicsScatteringHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyPosition and momentum space01 natural sciencesScattering amplitudeQuantum mechanics0103 physical sciencesMinkowski spaceCovariant transformation010306 general physicsPhysical Review D
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Structure of longitudinal chromomagnetic fields in high energy collisions

2014

We compute expectation values of spatial Wilson loops in the forward light cone of high-energy collisions. We consider ensembles of gauge field configurations generated from a classical Gaussian effective action as well as solutions of high-energy renormalization group evolution with fixed and running coupling. The initial fields correspond to a color field condensate exhibiting domain-like structure over distance scales of order the saturation scale. At later times universal scaling emerges at large distances for all ensembles, with a nontrivial critical exponent. Finally, we compare the results for the Wilson loop to the two-point correlator of magnetic fields.

We compute expectation values of spatial Wilson loops in the forward light cone of high-energy collisions. We consider ensembles of gauge field configurations generated from a classical Gaussian effective action as well as solutions of high-energy renormalization group evolution with fixed and running coupling. The initial like structure over distance scales of oder the saturation scale. At later times universal scaling emerges at large distances for all ensembles with a nontrivial critical exponent. Finally we compare the resulats for the Wilson loop to the two-point correlator of magnetic fields. (C) 2014 The Authors. Published by Elsevier BV This is an open access article under the CC BY licenseNuclear and High Energy PhysicsWilson loopLARGE NUCLEINuclear TheoryField (physics)FOS: Physical sciences114 Physical sciences01 natural sciencesColor-glass condensateRENORMALIZATION-GROUPNuclear Theory (nucl-th)GLUON DISTRIBUTION-FUNCTIONSHigh Energy Physics - Phenomenology (hep-ph)Light cone0103 physical sciencesSCATTERINGGauge theory010306 general physicsSMALL-XEffective actionPhysicsCORRELATORSta114010308 nuclear & particles physicsCOLOR GLASS CONDENSATERenormalization groupEVOLUTIONJIMWLK EQUATIONHigh Energy Physics - PhenomenologySATURATIONQuantum electrodynamicsCritical exponentPhysics Letters B
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Short range correlations in the weak decay of Lambda hypernuclei.

1995

The differences found in the relativistic and nonrelativistic methods used in the literature to account for short range nuclear correlations in the decay of \ensuremath{\Lambda} hypernuclei are analyzed. By means of a schematic microscopic model for the origin of correlations, the appropriate method to include them in nuclear processes is derived and is found to be the same one used in the nonrelativistic approach. The differences do not stem from relativistic effects but from the improper implementation of the correlations in the relativistic approach, which leads to several pathologies as shown in the paper. General formulas are given to evaluate the nonmesonic decay width of finite hyper…

Weak interactions (Nuclear physics)PhysicsEstructura nuclearNuclear and High Energy PhysicsParticle physicsRange (particle radiation)Nuclear TheoryInteraccions febles (Física nuclear)Carbon-12HyperonsLambda baryonLambdaPionHiperonsNuclear structureNuclear ExperimentNucleonRelativistic quantum chemistryRadioactive decayPhysical review. C, Nuclear physics
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Anomalous quartic gauge boson couplings at hadron colliders

2000

We analyze the potential of the Fermilab Tevatron and CERN Large Hadron Collider (LHC) to study anomalous quartic vector--boson interactions (photon photon Z Z) and (photon photon W+ W-). Working in the framework of SU(2)_L X U(1)_Y chiral Lagrangians, we study the production of photons pairs accompanied by (e+e-), (e nu), and jet pairs to impose bounds on these new couplings, taking into account the unitarity constraints. We compare our findings with the indirect limits coming from precision electroweak measurements as well as with presently available direct searches at LEPII. We show that the Tevatron Run II can provide limits on these quartic limits which are of the same order of magnitu…

Weak interactions (Nuclear physics)PhysicsNuclear and High Energy PhysicsParticle physicsGauge bosonLarge Hadron ColliderUnitarityAcceleradors de partículesElectron–positron annihilationElectroweak interactionHadronHigh Energy Physics::PhenomenologyInteraccions febles (Física nuclear)TevatronFOS: Physical sciencesPartícules (Física nuclear)Particle acceleratorsNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentFermilabParticle Physics - PhenomenologyParticles (Nuclear physics)
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Early warning for VHE gamma-ray flares with the ARGO-YBJ detector

2011

Detecting and monitoring emissions from flaring gamma-ray sources in the very-high-energy (VHE, > 100 GeV) band is a very important topic in gamma-ray astronomy. The ARGO-YBJ detector is characterized by a high duty cycle and a wide field of view. Therefore, it is particularly capable of detecting flares from extragalactic objects. Based on fast reconstruction and analysis, real-time monitoring of 33 selected VHE extragalactic sources is implemented. Flares exceeding a specific threshold are reported timely, hence enabling the follow-up observation of these objects using more sensitive detectors, such as Cherenkov telescopes. (C) 2011 Elsevier B.V. All rights reserved.

Wide field of viewNuclear and High Energy PhysicsMonitoringAstrophysics::High Energy Astrophysical PhenomenaARGO-YBJFlaring phenomenonVHE extragalactic sourceAstrophysicsSettore FIS/05 - Astronomia E AstrofisicaInstrumentationSorgenti VHE extragalatticheArgoCherenkov radiationPhysicsFenomeni transientiWarning systemDetectorSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayMonitoring Flaring PhenomenonAstronomyWide fieldDuty cycleAmpio campo di vistaFlaring phenomena VHE extragalactic sources Gamma Ray Bursts Large Field of view telescope ARGO-YBJGamma-ray burst
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Resolution of the ATLAS muon spectrometer monitored drift tubes in LHC Run 2

2019

The momentum measurement capability of the ATLAS muon spectrometer relies fundamentally on the intrinsic single-hit spatial resolution of the monitored drift tube precision tracking chambers. Optimal resolution is achieved with a dedicated calibration program that addresses the specific operating conditions of the 354 000 high-pressure drift tubes in the spectrometer. The calibrations consist of a set of timing offsets and drift time to drift distance transfer relations, and result in chamber resolution functions. This paper describes novel algorithms to obtain precision calibrations from data collected by ATLAS in LHC Run 2 and from a gas monitoring chamber, deployed in a dedicated gas fac…

Wire chambers (MWPCdrift tube13000 GeV-cmsPhysics::Instrumentation and DetectorsmuonsTracking (particle physics)01 natural sciences030218 nuclear medicine & medical imagingHigh Energy Physics - ExperimentSubatomär fysikMWPCHigh Energy Physics - Experiment (hep-ex)Gaseous detectors0302 clinical medicineWire chambersDrift tubesSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]tracking detectorProportional chambersmomentum resolutionInstrumentationImage resolutionMathematical Physicsdrift tubesPhysicsLarge Hadron ColliderDrift chamberstrack data analysisMuon spectrometersResolution (electron density)DetectorSettore FIS/01 - Fisica SperimentaleATLAS:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]Wire chambers (MWPC Thin-gap chambers drift chambers drift tubes proportional chambers etc)medicine.anatomical_structureCERN LHC Collproportional chambers etc)Gaseous detectors; Muon spectrometers; Particle tracking detectors (gaseous detectors); Wire chambers (MWPC thin-gap chambers drift chambers drift tubes proportional chambers etc)MDT chambersWire chambers (MWPC)LHCcolliding beams [p p]Particle Physics - Experimentp p: scatteringspectrometer [muon]Ciências Naturais::Ciências Físicas530 PhysicsParticle tracking detectors (Gaseous detectors):Ciências Físicas [Ciências Naturais]610FOS: Physical sciencesdrift chamber [muon]gas [monitoring]programming03 medical and health sciencesOpticsAtlas (anatomy)Muon spectrometer0103 physical sciencesCalibrationmedicinemuon: drift chamberGaseous detectorddc:610drift chambersHigh Energy Physicsspatial resolutionMuonScience & Technology010308 nuclear & particles physicsbusiness.industryhep-ex:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]Thin-gap chamberscalibrationmonitoring: gasExperimental High Energy Physicsbusinessp p: colliding beamsmuon: spectrometerexperimental results
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The Wide Field Imager of the International X-ray Observatory

2010

The International X-ray Observatory (IXO) will be a joint X-ray observatory mission by ESA, NASA and JAXA. It will have a large effective area (3 m 2 at 1.25 keV) grazing incidence mirror system with good angular resolution (5 arcsec at 0.1–10 keV) and will feature a comprehensive suite of scientific instruments: an X-ray Microcalorimeter Spectrometer, a High Time Resolution Spectrometer, an X-ray Polarimeter, an X-ray Grating Spectrometer, a Hard X-ray Imager and a Wide-Field Imager. The Wide Field Imager (WFI) has a field-of-view of 18 ft � 18 ft. It will be sensitive between 0.1 and 15 keV, offer the full angular resolution of the mirrors and good energy resolution. The WFI will be imple…

X ray astronomyNuclear and High Energy PhysicsInternational X-ray ObservatorySettore ING-INF/01 - Elettronicalaw.inventionImagingOpticsObservatorylawAngular resolutionInstrumentationSpectroscopyPhysicsActive Pixel SensorsezeleSpectrometerbusiness.industryAmplifierTransistorDetectorPolarimeterIXOOptoelectronicsbusinessDEPFETIXO; X ray astronomy; DEPFET; Active Pixel Sensor; Imaging; Spectroscopy
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EBIT diagnostics using X-ray spectra of highly ionized Ne

2003

We have carried out a detailed analysis of highly ionized neon spectra collected at the NIST EBIT using an NTD germanium X-ray microcalorimeter developed at the Harvard-Smithsonian Center for Astrophysics [Nucl. Instr. and Meth. A 444 (2000) 156]. Our attention was focused especially on the Ne IX He-like triplet to check electron density diagnostics through the intercombination/forbidden line ratio. We have investigated possible effects of the ion dynamics on the plasma emission line intensities, looking at the dependence of the count-rate and the charge state distribution on the electron beam energy and current. The temperature and spatial distribution of the neon ions, and hence the overl…

X-ray spectraNuclear and High Energy PhysicsElectron densityEBITChemistrySurfaces Coatings and Filmchemistry.chemical_elementFizikai tudományokSurfaces and InterfacesPlasmaIonNeonSettore FIS/05 - Astronomia E AstrofisicaTermészettudományokIonizationAstrophysical plasmaPhysics::Atomic PhysicsEmission spectrumAtomic physicsIonization of atomForbidden mechanismInstrumentationExcitation
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Developments for resonance ionization laser spectroscopy of the heaviest elements at SHIP

2016

Abstract The experimental determination of atomic levels and the first ionization potential of the heaviest elements ( Z ⩾ 100 ) is key to challenge theoretical predictions and to reveal changes in the atomic shell structure. These elements are only artificially produced in complete-fusion evaporation reactions at on-line facilities such as the GSI in Darmstadt at a rate of, at most, a few atoms per second. Hence, highly sensitive spectroscopic methods are required. Laser spectroscopy is one of the most powerful and valuable tools to investigate atomic properties. In combination with a buffer-gas filled stopping cell, the Radiation Detected Resonance Ionization Spectroscopy (RADRIS) techniq…

YtterbiumNuclear and High Energy Physics010308 nuclear & particles physicschemistry.chemical_elementInstrumental chemistry01 natural sciencesAtmospheric-pressure laser ionizationchemistryExcited state0103 physical sciencesPhysics::Atomic PhysicsNobeliumLaser-induced breakdown spectroscopyIonization energyAtomic physics010306 general physicsSpectroscopyInstrumentationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Searches for heavy neutrinos from Z decays

1992

We have searched for possible fourth family heavy neutrinos, pair produced in Z0 decays, in a sample of about 112 000 hadronic Z0 final states collected with the DELPHI detector. For all mixing matrix elements we exclude a new Dirac neutrino lighter than 44.5 GeV at a 95% confidence level, if the neutrino couples to the electron or muon family, and lighter than 44.0 GeV, if the neutrino couples to the tau family. Depending on the values of the mixing element and to which lepton family the neutrino couples, we obtain mass limits up to 46.2 GeV. For all mixing matrix elements we exclude a new Majorana neutrino lighter than 39.0 GeV, if it couples to the electron or the muon family, and lighte…

Z-PEAK; LEPTONS; RESONANCE; LIMITS; QUARKSNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaElectron–positron annihilationHadron01 natural sciencesNuclear physicsLIMITS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QUARKSNuclear Experiment010306 general physicsMixing (physics)PhysicsMuon010308 nuclear & particles physicsDirac (video compression format)High Energy Physics::PhenomenologyRESONANCEZ-PEAKMAJORANALEPTONSPhysique des particules élémentairesFísica nuclearHigh Energy Physics::ExperimentNeutrinoParticle Physics - ExperimentLepton
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