Search results for "Muon"

showing 10 items of 1376 documents

"Table 2" of "Measurement of the Collins and Sivers asymmetries on transversely polarised protons"

2007

The COLLINS asymmetry for positively charged hadrons as a function of Z.

POLInclusiveMathematics::Group TheoryMU+ P --> MU+ HADRON+ X160160PolarizationHigh Energy Physics::PhenomenologyNeutral CurrentDeep Inelastic ScatteringComputer Science::Symbolic ComputationHigh Energy Physics::ExperimentNuclear ExperimentMuon production
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"Table 1" of "Measurement of the Collins and Sivers asymmetries on transversely polarised protons"

2007

The COLLINS asymmetry for positively charged hadrons as a function of X.

POLInclusiveMathematics::Group TheoryMU+ P --> MU+ HADRON+ X160160PolarizationHigh Energy Physics::PhenomenologyNeutral CurrentDeep Inelastic ScatteringComputer Science::Symbolic ComputationHigh Energy Physics::ExperimentNuclear ExperimentMuon production
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"Table 2" of "Measurement of the Antilambda polarization in nu/mu charged current interactions in the NOMAD experiment."

1993

Lambdabar polarization in regions of the Bjorken scaling variable X.

POLInclusiveNUMU NUCLEON --> MU- LAMBDABAR XStrange productionPolarizationDeep Inelastic ScatteringCharged CurrentMuon production0.938-29.07
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"Table 1" of "Measurement of the Antilambda polarization in nu/mu charged current interactions in the NOMAD experiment."

1993

Lambdabar polarization in regions of Feynman X (XL).

POLInclusiveNUMU NUCLEON --> MU- LAMBDABAR XStrange productionPolarizationDeep Inelastic ScatteringHigh Energy Physics::ExperimentCharged Current31.872Muon production
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Search for doubly charged higgs bosons with lepton-rlavor-violating decays involving τ leptons

2008

We search for pair production of doubly charged Higgs particles (H(+/-+/-)) followed by decays into electron-tau (e tau) and muon-tau (mu tau) pairs using data (350 pb(-1)) collected from (p) over barp collisions at root s = 1.96 TeV by the CDF II experiment. We search separately for cases where three or four final-state leptons are detected, and combine results for exclusive decays to left-handed e tau (mu tau) pairs. We set an H(+/-+/-) lower mass limit of 114(112) GeV/c(2) at the 95% confidence level. RI Ruiz, Alberto/E-4473-2011; Robson, Aidan/G-1087-2011; De Cecco, Sandro/B-1016-2012; Prokoshin, Fedor/E-2795-2012; Azzi, Patrizia/H-5404-2012

Pair productionParticle physicsGeneral Physics and AstronomyFOS: Physical sciencesElementary particleddc:500.201 natural sciencesHigh Energy Physics - ExperimentNuclear physicsTellurium compoundsParticle decayHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesHiggs particles010306 general physicsBosonsBosonPhysicsHiggs bosonsMuon010308 nuclear & particles physicsBranching fractionPhysicsHigh Energy Physics::PhenomenologyPair productionConfidence levelHiggs boson_High Energy Physics::ExperimentLepton
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Hysteresis in the spin transition regime of [Fe(NH2trz)3](NO3)2 as probed by ZF-μSR

2006

The thermal spin transition which occurs in the polymeric chain compound [Fe(NH(2)trz)(3)](NO3)(2) above room temperature has been investigated by zero-field muon spin relaxation (mu SR) (similar to 8-402 K). The depolarization curves are best described by a Lorentzian and a Gaussian line that represent fast and slow components respectively. The spin transition is associated with a hysteresis loop of width Delta T = 34 K (T-1/2(up arrow) = 346 K and T-1/2(down arrow) = 312 K) that has been delineated by the temperature variation of the initial asymmetry parameter. Comparison of zero-field and transverse field (20 Oe) mu SR measurements shows that diamagnetic muon species occur over the enti…

ParamagnetismMaterials scienceMuonCondensed matter physicsSpin crossoverRelaxation (NMR)MuoniumSpin transitionElectrical and Electronic EngineeringAtmospheric temperature rangeMuon spin spectroscopyCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsPhysica B: Condensed Matter
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The energy spectrum of atmospheric neutrinos between 2 and 200 TeV with the AMANDA-II detector

2010

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2 - 200 TeV. The result is compared to different atmospheric neutrino models and it is compatible with the atmospheric neutrinos from pion and kaon decays. No significant contribution from charm hadron decays or extraterrestrial neutrinos is detected. The capabilities to improve the measurement of the neutrino spectrum with the successor experiment IceCube are discussed.

Particle physicsAMANDA[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Solar neutrinoAstrophysics::High Energy Astrophysical PhenomenaAMANDA; Atmospheric neutrinos; Cherenkov radiation; Neural net; Unfoldingneural netFOS: Physical sciencesAetiology screening and detection [ONCOL 5]01 natural sciences7. Clean energy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsunfoldingPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cherenkov radiationHigh Energy Physics::PhenomenologyAstronomy and AstrophysicsSolar neutrino problematmospheric neutrinosCosmic neutrino backgroundNeutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Inclusive semileptonic branching ratios of b hadrons produced in Z decays

2001

A measurement of the inclusive semileptonic branching ratios of b hadrons produced in Z decay is presented, using four million hadronic events collected by the ALEPH detector from 1991 to 1995. Electrons and muons are selected opposite to b-tagged hemispheres. Two different methods are explored to distinguish the contributions from direct $\bl$ and cascade $\bcl$ decays to the total lepton yield. One is based on the lepton transverse momentum spectrum, the other makes use of the correlation between the charge of the lepton and charge estimators built from tracks in the opposite hemisphere of the event. The latter method reduces the dependence on the modelling of semileptonic b decays. The r…

Particle physicsAleph[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]Physics and Astronomy (miscellaneous)MesonElectron–positron annihilationHadronFOS: Physical sciencesElectron7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsEngineering (miscellaneous)PhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCascadeHigh Energy Physics::ExperimentParticle Physics - ExperimentLeptonThe European Physical Journal C
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Measurement of the Charged-Pion Polarizability

2015

The COMPASS collaboration at CERN has investigated pion Compton scattering, $\pi^-\gamma\rightarrow \pi^-\gamma$, at centre-of-mass energy below 3.5 pion masses. The process is embedded in the reaction $\pi^-\mathrm{Ni}\rightarrow\pi^-\gamma\;\mathrm{Ni}$, which is initiated by 190\,GeV pions impinging on a nickel target. The exchange of quasi-real photons is selected by isolating the sharp Coulomb peak observed at smallest momentum transfers, $Q^2<0.0015$\,(GeV/$c$)$^2$. From a sample of 63\,000 events the pion electric polarisability is determined to be $\alpha_\pi\ =\ (\,2.0\ \pm\ 0.6_{\mbox{\scriptsize stat}}\ \pm\ 0.7_{\mbox{\scriptsize syst}}\,) \times 10^{-4}\,\mbox{fm}^3$ under the …

Particle physicsChiral perturbation theoryPhotonComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATIONStrong interactionComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONGeneral Physics and AstronomyFOS: Physical sciencesComputerApplications_COMPUTERSINOTHERSYSTEMSGeneralLiterature_MISCELLANEOUSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionPolarizabilityNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentPhysicsChPTMuonCompton scatteringpolarisabilitypolarisability; ChPTComputingMethodologies_PATTERNRECOGNITIONHigh Energy Physics::ExperimentMagnetic dipoleParticle Physics - Experiment
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Multi-PeV Signals from a New Astrophysical Neutrino Flux beyond the Glashow Resonance.

2016

The IceCube neutrino discovery was punctuated by three showers with $E_\nu$ ~ 1-2 PeV. Interest is intense in possible fluxes at higher energies, though a marked deficit of $E_\nu$ ~ 6 PeV Glashow resonance events implies a spectrum that is soft and/or cutoff below ~few PeV. However, IceCube recently reported a through-going track event depositing 2.6 $\pm$ 0.3 PeV. A muon depositing so much energy can imply $E_{\nu_\mu} \gtrsim$ 10 PeV. We show that extending the soft $E_\nu^{-2.6}$ spectral fit from TeV-PeV data is unlikely to yield such an event. Alternatively, a tau can deposit this much energy, though requiring $E_{\nu_\tau}$ ~10x higher. We find that either scenario hints at a new flu…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesCosmic ray01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Flux (metallurgy)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics - Astrophysics of GalaxiesHigh Energy Physics - PhenomenologyAstrophysics of Galaxies (astro-ph.GA)High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)Energy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical review letters
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