Search results for "positron"

showing 10 items of 1346 documents

Measurement of Z-pair production in e(+)e(-) collisions and constraints on anomalous neutral gauge couplings

2009

The ZZ production cross section is measured from a data sample corresponding to a total integrated luminosity of 452 pb−1, collected by the ALEPH experiment at LEP at centre-of-mass energies from 192 to 209 GeV. Individual cross sections, extracted at six centre-of-mass energies, are found to be in agreement with Standard Model calculations. The results are used to set limits on anomalous neutral gauge couplings. The ZZ production cross section is measured from a data sample corresponding to a total integrated luminosity of 452 pb−1 , collected by the ALEPH experiment at LEP at centre-of-mass energies from 192 to 209 GeV. Individual cross sections, extracted at six centre-of-mass energies, …

PhysicsAlephParticle physicsNuclear and High Energy PhysicsLuminosity (scattering theory)e+-e- Experiments010308 nuclear & particles physicsElectron–positron annihilationSettore FIS/01 - Fisica SperimentaleGauge (firearms)01 natural sciencesStandard ModelNuclear physicsE +e -experiments; Nuclear and High Energy PhysicsE +e -experimentsCross section (physics)Pair production0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::Experiment010306 general physicsALEPH experimentParticle Physics - Experiment
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Transverse momentum correlations in hadronic Z decays

1997

Using data obtained with the ALEPH detector at the Z resonance, a measure based on transverse momentum is shown to exhibit a correlation between the two halves of a hadronic event which cannot be explained by energy-momentum conservation, flavour conservation, the imposition of an event axis or imperfect event reconstruction. Two possible interpretations based on existing Monte Carlo models are examined: a) ARIADNE, with the correlation forming early in the parton shower and with the transition from partons to hadrons playing only a minor part; b) JETSET, with the correlation forming at the fragmentation stage. A correlation technique based on a jet cluster analysis is used to make a compar…

PhysicsAlephParticle physicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsPhysicsElectron–positron annihilationDetectorMonte Carlo methodHadronParton01 natural sciencesNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentNuclear Experiment010306 general physicsParton showerParticle Physics - ExperimentEvent reconstructionZeitschrift f�r Physik C Particles and Fields
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Measurement of higher-order multipole amplitudes in ψ(3686)→γχc1,2 with χc1,2→γJ/ψ and search for the transition ηc(2S)→γJ/ψ

2017

Using 106 x 10(6) psi(3686) events collected with the BESIII detector, we measure multipole amplitudes for the decay psi(3686) ->; gamma chi(c1,2) -> gamma gamma J/psi beyond the dominant electric-dipole amplitudes. The normalized magnetic-quadrupole (M2) amplitude for psi(3686) -> gamma chi(c1,2) -> gamma gamma J/psi and the normalized electric-dipole amplitudes for psi(3686) -> gamma chi(c2) -> gamma J/psi and determined. The M2 amplitudes for psi(3686) -> gamma chi(c1) and ; chi(c1,2) -> gamma J/psi are found to differ significantly from zero and are consistent with theoretical predictions. We also obtain the ratios of M2 contributions of psi(3686) and J/psi decays to;2,chi(c1,2,) b(2)(1…

PhysicsAmplitude010308 nuclear & particles physicsBranching fractionAstrophysics::High Energy Astrophysical PhenomenaElectron–positron annihilation0103 physical sciencesAnalytical chemistryHigh Energy Physics::Experiment010306 general physicsMultipole expansion01 natural sciencesGamma gammaPhysical Review D
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Galactic synchrotron emission from WIMPs at radio frequencies

2011

Dark matter annihilations in the Galactic halo inject relativistic electrons and positrons which in turn generate a synchrotron radiation when interacting with the galactic magnetic field. We calculate the synchrotron flux for various dark matter annihilation channels, masses, and astrophysical assumptions in the low-frequency range and compare our results with radio surveys from 22 MHz to 1420 MHz. We find that current observations are able to constrain particle dark matter with "thermal" annihilation cross-sections, i.e. (\sigma v) = 3 x 10^-26 cm^3/s, and masses M_DM < 10 GeV. We discuss the dependence of these bounds on the astrophysical assumptions, namely galactic dark matter distribu…

PhysicsAnnihilation010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesSynchrotron radiationAstronomy and AstrophysicsCosmic rayAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesAstrophysics - Astrophysics of GalaxiesSynchrotronlaw.inventionGalactic haloPositronlawAstrophysics of Galaxies (astro-ph.GA)0103 physical sciences010303 astronomy & astrophysics
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Evidence for the Rare DecayB+→Ds+π0

2007

We have searched for the rare decay B+ -> D-s(+) pi(0). The analysis is based on a sample of 232 X 10(6) Y(4S) -> B (B) over bar decays collected with the BABAR detector at the SLAC PEP-II e(+)e(-) storage ring. We find 19.6 signal events, corresponding to a significance of 4.7 sigma. The extracted signal yield including statistical and systematic uncertainties is 20.1(-6.0-1.5)(+6.8+0.4) and we measure B(B+ -> D-s(+) pi(0)) = (1.5(-0.4)(+0.5) +/- 0.1 +/- 0.2) X x 10(-5), where the first uncertainty is statistical, the second is systematic, and the last is due to the uncertainty on the D-s(+) decay and its daughter decay branching fractions.

PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionElectron–positron annihilationAnalytical chemistryGeneral Physics and Astronomy01 natural sciencesNuclear physicsParticle decayYield (chemistry)0103 physical sciencesPiB meson010306 general physicsBar (unit)Physical Review Letters
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Measurement of the Pseudoscalar Decay ConstantfDsUsing Charm-Tagged Events ine+e−Collisions ats=10.58  GeV

2007

Using 230.2 fb^(-1) of e+e- annihilation data collected with the BABAR detector at and near the peak of the Y(4S) resonance, 489 +/- 55 events containing the pure leptonic decay D_s^+ --> mu^+ nu_mu have been isolated in charm-tagged events. The ratio of partial widths Gamma(D_s^+ --> mu^+ nu_mu)/Gamma(D_s^+ --> phi pi^+) is measured to be 0.143 +/- 0.018 +/- 0.006 allowing a determination of the pseudoscalar decay constant f_{D_s} = (283 +/- 17 +/- 7 +/- 14) MeV. The errors are statistical, systematic, and from the D_s^+ --> phi pi^+ branching ratio, respectively.

PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionElectron–positron annihilationGeneral Physics and AstronomyResonanceElectron01 natural sciencesNuclear physicsPseudoscalarPositron0103 physical sciencesExponential decay010306 general physicsPhysical Review Letters
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Measurement of the Branching Fraction and Photon Energy Moments ofB→XsγandACP(B→Xs+dγ)

2006

The photon spectrum in B -> X-s gamma decay, where X-s is any strange hadronic state, is studied using a data sample of 88.5x10(6) e(+)e(-)->Upsilon(4S)-> B(B) over bar decays collected by the BABAR experiment at the Stanford Linear Accelerator Center. The partial branching fraction, Delta B(B -> X-s gamma)=(3.67 +/- 0.29(stat)+/- 0.34(syst)+/- 0.29(model))x10(-4), the first moment =2.288 +/- 0.025 +/- 0.017 +/- 0.015 GeV, and the second moment =0.0328 +/- 0.0040 +/- 0.0023 +/- 0.0036 GeV2 are measured for the photon energy range 1.9 GeV 1.6 GeV. In addition, the direct CP asymmetry A(CP)(B -> Xs+d gamma) is measured to be -0.110 +/- 0.115(stat)+/- 0.017(syst).

PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionElectron–positron annihilationHadronGeneral Physics and AstronomyPhoton energy01 natural sciencesNuclear physicsParticle decay0103 physical sciencesCP violationB meson010306 general physicsPhysical Review Letters
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Measurement of the Absolute Branching Fraction forΛc+→Λe+νe

2015

We report the first measurement of the absolute branching fraction for Lambda(+)(c) -> Lambda e(+)nu(e). This measurement is based on 567 pb(-1) of e(+)e(-) annihilation data produced at root s = 4.599 GeV, which is just above the Lambda(+)(c)Lambda(-)(c) threshold. The data were collected with the BESIII detector at the BEPCII storage rings. The branching fraction is determined to be B(Lambda(+)(c) -> Lambda e(+)nu(e)) = [3.63 +/- 0.38(stat) +/- 0.20(syst)] %, representing a significant improvement in precision over the current indirect determination. As the branching fraction for Lambda(+)(c) -> Lambda e(+)nu(e) is the benchmark for those of other Lambda(+)(c) semileptonic channels, our r…

PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionElectron–positron annihilationTheoretical modelsAnalytical chemistryGeneral Physics and AstronomyLambda baryonLambda01 natural sciencesNuclear physicsBaryonCharmed baryons0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsPhysical Review Letters
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Positron Annihilation Characteristics in Superstrong Magnetic Fields

2010

The recent interest in positrons distribution in the space revealed the anomalous presence of high energetic positrons. There are different possible origins of such positrons, including the decay of heavy particles in the dark matter, also pulsars or neutron stars. In our study we calculated the annihilation properties of the electron – positron bound system in superstrong magnetic fields expected for neutron stars. For this aim we use solutions of the (relativistic) Bethe-Salpeter equation derived by L.B. Leinson and A. Perez [1]. The results indicate strong dependency of the annihilation properties (rate and intensity) on the value of the magnetic field.

PhysicsAnnihilationAstrophysics::High Energy Astrophysical PhenomenaMechanical EngineeringDark matterElectronCondensed Matter PhysicsPositroniumMagnetic fieldNuclear physicsNeutron starPositronPulsarMechanics of MaterialsGeneral Materials ScienceAtomic physicsMaterials Science Forum
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Atomic physics of positronium with intense slow positron beams

2002

Abstract The theory of quantum electrodynamics has presented a complete calculation of the energy levels of positronium (Ps, e + e − ) up to the order R ∞ α 4 . The annihilation rates for para -Ps (1 1 S 0 ) and ortho -Ps (1 1 S 1 ) are completely known up to the order R ∞ α 5 and R ∞ α 6 , respectively. The present experimental uncertainty for spectroscopic results is 5–100 times larger than the theoretical uncertainty. For the annihilation rates the experimental situation is even worse. The theoretical predictions have presently reached a level of precision which is a challenge to experimentalists! The experimental uncertainty for the fine- and hyperfine transitions in the Ps atom is dete…

PhysicsAnnihilationBremsstrahlungGeneral Physics and AstronomySurfaces and InterfacesGeneral ChemistryElectronCondensed Matter PhysicsSurfaces Coatings and Filmslaw.inventionPositroniumNuclear physicsPositronlawAtomBeam dumpAtomic physicsHyperfine structureApplied Surface Science
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