Search results for "nuclear physics"

showing 10 items of 5307 documents

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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Applications of light-matter interaction in nanosciences

2009

In this thesis, light matter interaction in nanoscale has been studied from various aspects. The interaction between surface plasmon polaritons (SPPs) and optically active organic molecules (Rhodamine 6G, Sulforhodamine 101 and Coumarine 30) and semiconducting nanocrystals (quantum dots) is studied in the weak coupling regime. In particular, a photon-SPP-photon conversion with spatially separated inand outcoupling was demonstrated by using molecules. Also, a frequency downconversion for propagating SPPs was presented by utilization of vibrational relaxation of organic molecules. A strong coupling regime was reached for Rhodamine 6G (R6G) and SPP despite the broad absorption linewidth of R6G…

Weak interactions (Nuclear physics)Quantum dotssurface plasmon polaritonsStrong interactions (Nuclear physics)Physics::OpticsPolaritonsBose-Einstein condensationMoleculesnanotieteetPlasmons (Physics)pattern transfer
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Centrality-dependent forward J/ψ production in high energy proton-nucleus collisions

2016

Forward $J/\psi$ production and suppression in high energy proton-nucleus collisions can be an important probe of gluon saturation. In an earlier work we studied this process in the Color Glass Condensate framework and showed that using the Glauber approach to extrapolate the dipole cross section of a proton to a nucleus leads to results closer to experimental data than previous calculations in this framework. Here we investigate the centrality dependence of the nuclear suppression in this model and show a comparison of our results with recent LHC data.

Work (thermodynamics)Particle physicshigh energyNuclear TheoryProtonQC1-999Nuclear Theory114 Physical sciences01 natural sciences7. Clean energyColor-glass condensateNuclear physics0103 physical sciencesmedicineproton-nucleus collisionsNuclear Experiment010306 general physicsPhysicsLarge Hadron Colliderta114010308 nuclear & particles physicsPhysicsGluonHigh Energy Physics - PhenomenologyDipolemedicine.anatomical_structureJ/ψ productionNucleusGlauberInternational Conference on Physics Opportunities at an Electron-Ion Collider
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Collinear fast-beam laser spectroscopy

1987

The progress in atomic and molecular spectroscopy has gone hand in hand with improvements of the resolution. Before the tunable narrow-band lasers led to the invention of Doppler-free techniques, spectral lines from cooled hollow-cathode discharges(1) had typical widths larger than 300 MHz, and high resolution was achieved only in rf spectroscopy, e.g., within hyperfine structure multiplets, by the classical techniques like atomic beam magnetic resonance,(2) optical pumρing,(3) or double resonance.(4) While the Doppler broadening $$\delta {v_D} = {v_0}{\left( {{{8kT{\rm{ }}\ln {\rm{ 2}}} \over {m{c^2}}}} \right)^{1/2}}$$ (1) is negligible for resonance frequencies v 0 in the rf regime, the …

X-ray laserPhysicsThermal velocityResonanceNuclear Physics - ExperimentAtomic physicsCoherent spectroscopySpectroscopyHyperfine structureSpectral lineDoppler broadening
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First Dark Matter Search Results from the XENON1T Experiment

2017

We report the first dark matter search results from XENON1T, a ∼2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042±12)-kg fiducial mass and in the [5,40] keVnr energy range of interest for weakly interacting massive particle (WIMP) dark matter searches, the electronic recoil background was (1.93±0.25)×10-4 events/(kg×day×keVee), the lowest ever achieved in such a dark matter detector. A profile likelihood analysis shows that the data are consisten…

Xenon[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Massive particleGeneral Physics and Astronomy01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)RecoilXenonWIMPS046DM2[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matter[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]PhysicsRange (particle radiation)Time projection chamberDetectorHigh Energy Physics - Phenomenologydark matter: scatteringTPCAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPDark matterFOS: Physical scienceschemistry.chemical_elementWIMP: massS030DI2Nuclear physicsPhysics and Astronomy (all)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesrecoil[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physique010308 nuclear & particles physicsbackgrounddark matter: detectorAstronomieGran SassochemistryDirect Searchtime projection chamber: xenoninterpretation of experiments: XENON[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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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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Electron and photon energy calibration with the ATLAS detector using 2015-2016 LHC proton-proton collision data

2019

Artículo realizado por muchos autores. Solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración y los autores que firman como pertenecientes a la UAM

Z0 --> electron positronJ/psi(3100) --> electron positronProton13000 GeV-cmsparticle identification [electron]ElectronZ0 --> electron positronelectron: transverse momentum01 natural sciencesphoton: particle identificationSubatomär fysik0302 clinical medicinescattering [p p]Nuclear Experiment proton–proton collisionsLarge Hadron ColliderCalibration and fittingphoton: transverse momentumand fitting methodsphoton: energy:Mathematics and natural scienses: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]calibration [energy]CERN LHC Collcalibration and fitting methodcolliding beams [p p]transverse momentum [electron]p p: scatteringCiências Naturais::Ciências Físicas610LHC ATLAS High Energy PhysicsPhoton energyFitting methodsJ/psi(3100) --> electron positronradiative decay [J/psi(3100)]Nuclear physicsMomentum03 medical and health sciencesAtlas (anatomy)High Energy Physicspair production [electron]CALORIMETERScience & Technologyradiative decay [Z0]electron: particle identification010308 nuclear & particles physicsenergy [photon]Acceleratorfysik och instrumentering jets energy: calibrationCalorimeter methodExperimental High Energy PhysicsPerformance of High Energy Physics Detectorsp p: colliding beamsacceptancetransverse momentum [photon]PhotonJ/psi(3100): radiative decayCalorimeter methods; Pattern recognition cluster finding calibration; and fitting methods; Performance of High Energy Physics Detectors; PARTON DISTRIBUTIONS; LIQUID AR; CALORIMETER; KR030218 nuclear medicine & medical imagingHigh Energy Physics - Experimentelectron: pair productionHigh Energy Physics - Experiment (hep-ex)Subatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Collisions Calorimeter methodsInstrumentationMathematical PhysicsBosonPhysicsPattern recognition cluster finding calibration and fitting methodsSettore FIS/01 - Fisica Sperimentalecalibration and fitting methodsATLASLIQUID ARmedicine.anatomical_structureKRCalibrationcalibration and fitting methods; Calorimeter methods; cluster finding; Pattern recognition; Performance of High Energy Physics Detectors; Instrumentation; Mathematical PhysicsParticle Physics - Experiment530 Physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesZ0: radiative decayAccelerator Physics and Instrumentationcalibration and fitting methods; Calorimeter methods; cluster finding; Pattern recognition; Performance of High Energy Physics DetectorsPattern recognition0103 physical sciencesmedicineddc:610hep-exCluster finding:Matematikk og naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431 [VDP]particle identification [photon]FísicaPARTON DISTRIBUTIONSHigh Energy Physics::Experimentexperimental results
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Interpretation of the depths of maximum of extensive air showers measured by the Pierre Auger Observatory

2013

To interpret the mean depth of cosmic ray air shower maximum and its dispersion, we parametrize those two observables as functions of the first two moments of the ln A distribution. We examine the goodness of this simple method through simulations of test mass distributions. The application of the parameterization to Pierre Auger Observatory data allows one to study the energy dependence of the mean ln A and of its variance under the assumption of selected hadronic interaction models. We discuss possible implications of these dependences in term of interaction models and astrophysical cosmic ray sources.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Ciencias FísicasAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesCosmic rayultra high energy cosmic rays01 natural sciencesultra high energy cosmic rayInterpretation (model theory)//purl.org/becyt/ford/1 [https]Nuclear physics0103 physical sciencesPARTICLES010306 general physicsDispersion (water waves)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryCOMPOSICIÓN DE MASAEXPERIMENTO AUGER010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsObservableASTROFÍSICA//purl.org/becyt/ford/1.3 [https]RAYOS COSMICOSAstronomíaENERGY COSMIC-RAYSMODELDistribution (mathematics)Air showerParticlesUltra High Energy Cosmic RaysExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGEnergy cosmic-raysFísica nuclearcosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASSimulationcosmic ray experiments; ultra high energy cosmic raysModel
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Measurement of the Depth of Maximum of Extensive Air Showers above 10(18) eV

2010

We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost four thousand events above 10¹⁸ eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106⁺³⁵₋₂₁) g/cm²/decade below 1018.24 ± 0.05 eV and (24 ± 3) g/cm²/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm². The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FLUORESCENCE LIGHTGeneral Physics and AstronomyPierre Auger Observatory; depth of maximum; fluorescence detector; cosmic raysFOS: Physical sciencesCosmic rayChemical CompositionAstrophysicsMass compositionENERGIA01 natural sciencesCoincidenceAugerNuclear physicsPhysics and Astronomy (all)cosmic rays0103 physical sciencesRECONSTRUCTIONHigh-Energy Cosmic Ray010303 astronomy & astrophysicsDETECTORCiencias ExactasPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MeasurementSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ExperimentDetectorPrimary compositionFísicaPierre Auger ObservatoryCOSMIC-RAYSCosmic raylongitudinal developmentLongitudinal developmentRESOLUTIONFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenaenergyPhysical Review Letters
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