Search results for "SPECTRA"

showing 10 items of 3542 documents

Steady-State X-Ray Radiation-Induced Attenuation in Canonical Optical Fibers

2020

The so-called canonical optical fibers (OFs) are samples especially designed to highlight the impact of some manufacturing process parameters on the radiation responses. Thanks to the results obtained on these samples, it is thus possible to define new procedures to better control the behaviors of OFs in radiation environments. In this article, we characterized the responses, under steady-state X-rays, of canonical samples representative of the most common fiber types differing by their core-dopants: pure silica, Ge, Al, and P. Their radiation-induced attenuation (RIA) spectra were measured online at both room temperature (RT) and liquid nitrogen temperature (LNT), in the energy range [~0.6…

Nuclear and High Energy PhysicsOptical fiberMaterials scienceDoped optical fibers)Analytical chemistryRadiation01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencespoint defectsFiberIrradiationElectrical and Electronic EngineeringAbsorption (electromagnetic radiation)ComputingMilieux_MISCELLANEOUSpure silica core[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]010308 nuclear & particles physicsAttenuationSettore FIS/01 - Fisica SperimentaleX-rayAttenuationNuclear Energy and Engineeringradiation effects
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Radiation effects on silica-based preforms and optical fibers-I: Experimental study with canonical samples

2008

International audience; Prototype samples of preforms and associated fibers have been designed and fabricated through MCVD process to investigate the role of fluorine (F) and germanium (Ge) doping elements on the radiation sensitivity of silica-based glasses. We characterized the behaviors of these canonical samples before, during and after 10 keV X-ray irradiation through several spectroscopic techniques, to obtain global information (in situ absorption measurements, electron paramagnetic resonance) or spatially-resolved information (confocal microscopy, absorption and luminescence on preform). These tests showed that, for the Ge-doped fiber and in the 300–900 nm range, the radiation-induc…

Nuclear and High Energy PhysicsOptical fiberMaterials scienceoptical fibersAnalytical chemistrychemistry.chemical_elementGermanium02 engineering and technologyconfocal microscopy01 natural sciencesSpectral linelaw.inventionAbsorptionX-rays.law0103 physical sciencesX-raysluminescencepoint defectsIrradiationFiberElectrical and Electronic EngineeringAbsorption (electromagnetic radiation)010302 applied physics[PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]021001 nanoscience & nanotechnologyCrystallographic defectOptical fiber photosensitivity absorption luminescenceNuclear Energy and EngineeringchemistryEPR0210 nano-technologyLuminescence
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The cosmic ray proton plus helium energy spectrum measured by the ARGO-YBJ experiment in the energy range 3-300 TeV

2015

The ARGO-YBJ experiment is a full-coverage air shower detector located at the Yangbajing Cosmic Ray Observatory (Tibet, People's Republic of China, 4300 m a.s.l.). The high altitude, combined with the full-coverage technique, allows the detection of extensive air showers in a wide energy range and offer the possibility of measuring the cosmic ray proton plus helium spectrum down to the TeV region, where direct balloon/space-borne measurements are available. The detector has been in stable data taking in its full configuration from November 2007 to February 2013. In this paper the measurement of the cosmic ray proton plus helium energy spectrum is presented in the region 3-300 TeV by analyzi…

Nuclear and High Energy PhysicsPARTICLE-ACCELERATIONPhysics and Astronomy (miscellaneous)ProtonAstrophysics::High Energy Astrophysical PhenomenaSHELLFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesUltra-high-energy cosmic ray010306 general physicsCosmic-ray observatoryDETECTORNuclear and High Energy PhysicPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSSpectral index010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsSpectral densityAir shower13. Climate actionSUPERNOVA REMNANTHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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Spectral analysis of the high-energy IceCube neutrinos

2015

A full energy and flavor-dependent analysis of the three-year high-energy IceCube neutrino events is presented. By means of multidimensional fits, we derive the current preferred values of the high-energy neutrino flavor ratios, the normalization and spectral index of the astrophysical fluxes, and the expected atmospheric background events, including a prompt component. A crucial assumption resides on the choice of the energy interval used for the analyses, which significantly biases the results. When restricting ourselves to the ~30 TeV - 3 PeV energy range, which contains all the observed IceCube events, we find that the inclusion of the spectral information improves the fit to the canoni…

Nuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesMuon neutrino010306 general physicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral indexMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGlashow resonanceFísicaSpectral densitySolar neutrino problemHigh Energy Physics - Phenomenology13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Multiplicity dependence of mean transverse momentum in $e^+e^-$ annihilations at LEP energies

1992

A strong increase of the mean transverse momentum [p(t)] with the number of charged particles n(ch) is observed in e+e- annihilations into hadrons at LEP energies, The effect resembles correlations observed in hadron-hadron interactions. In e+e- annihilations the [p(t)] and n(ch) correlations can be accounted for by gluon radiation.

Nuclear and High Energy PhysicsParticle physicsCOLLISIONSElectron–positron annihilationHadronNuclear TheoryISR ENERGIESANTI-PROTON COLLIDER; ISR ENERGIES; COLLISIONS; SPECTRA; EVENTS; MATTER; QCDRadiation01 natural sciencesANTI-PROTON COLLIDERNuclear physicsEVENTS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SPECTRAMultiplicity (chemistry)010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyQCDCharged particleGluonTransverse momentumFísica nuclearHigh Energy Physics::ExperimentMATTERParticle Physics - Experiment
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On the pion cloud of the nucleon

2003

We evaluate the two--pion contribution to the nucleon electromagnetic form factors by use of dispersion analysis and chiral perturbation theory. After subtraction of the rho--meson component, we calculate the distributions of charge and magnetization in coordinate space, which can be interpreted as the effects of the pion cloud. We find that the charge distribution of this pion cloud effect peaks at distances of about 0.3 fm. Furthermore, we calculate the contribution of the pion cloud to the isovector charges and radii of the nucleon.

Nuclear and High Energy PhysicsParticle physicsChiral perturbation theoryNuclear Theorydispersion relationHigh Energy Physics::LatticeisovectorNuclear Theorychiral [perturbation theory]FOS: Physical sciencestwo-pion [effect]form factor [nucleon]density [charge]Nuclear physicsNuclear Theory (nucl-th)PionHigh Energy Physics - Phenomenology (hep-ph)ddc:530Perturbation theoryCoordinate spacenumerical calculationsNuclear ExperimentPhysicsIsovectorpole [rho(770)]Charge densityCharge (physics)High Energy Physics - Phenomenologycloud [pi]High Energy Physics::Experimentspectral representationNucleon
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Probing neutrino masses with CMB lensing extraction

2005

We evaluate the ability of future cosmic microwave background (CMB) experiments to measure the power spectrum of large scale structure using quadratic estimators of the weak lensing deflection field. We calculate the sensitivity of upcoming CMB experiments such as BICEP, QUaD, BRAIN, ClOVER and PLANCK to the non-zero total neutrino mass M_nu indicated by current neutrino oscillation data. We find that these experiments greatly benefit from lensing extraction techniques, improving their one-sigma sensitivity to M_nu by a factor of order four. The combination of data from PLANCK and the SAMPAN mini-satellite project would lead to sigma(M_nu) = 0.1 eV, while a value as small as sigma(M_nu) = 0…

Nuclear and High Energy PhysicsParticle physicsCosmic microwave backgroundDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesPlanckNeutrino oscillation010303 astronomy & astrophysicsWeak gravitational lensingPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsFísicaSpectral densityHigh Energy Physics - PhenomenologyDark energysymbolsNeutrino
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Reliability of Monte Carlo event generators for gamma-ray dark matter searches

2013

We study the differences in the gamma-ray spectra simulated by four Monte Carlo event generator packages developed in particle physics. Two different versions of PYTHIA and two of HERWIG are analyzed, namely PYTHIA 6.418 and HERWIG 6.5.10 in Fortran and PYTHIA 8.165 and HERWIG 2.6.1 in C++. For all the studied channels, the intrinsic differences between them are shown to be significative and may play an important role in misunderstanding dark matter signals.

Nuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FortranMonte Carlo methodDark matterFOS: Physical sciencesGamma ray spectra01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Reliability (semiconductor)0103 physical sciences010303 astronomy & astrophysicsEvent generatorcomputer.programming_languageHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGamma rayFísicaHigh Energy Physics - PhenomenologyMonte Carlo SimulationsAstrophysics - High Energy Astrophysical PhenomenacomputerEvent (particle physics)Astrophysics - Cosmology and Nongalactic Astrophysics
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Energy dependence of inclusive spectra in e+ e- annihilation

1999

Inclusive charged hadron distributions as obtained from the DELPHI measurements at 130, 136, 161, 172 and 183 GeV are presented as a function of the variables rapidity, xi(p), p and transversal momenta. Data are compared with event generators and with MLLA calculations, in order to examine the hypothesis of local parton hadron duality. The differential momentum spectra show an indication for coherence effects in the production of soft particles. The relation between the energy dependence of the charged multiplicity and the rapidity distribution is examined. (C) 1999 Elsevier Science B.V. All rights reserved.

Nuclear and High Energy PhysicsParticle physicsE+E ANNIHILATIONElectron–positron annihilationHadronParton01 natural sciencesCHARGED-PARTICLE MULTIPLICITY; QCD JETS; E+E ANNIHILATION; FRAGMENTATION; EVENTSSpectral lineQCD JETSEVENTSNuclear physics0103 physical sciencesCHARGED-PARTICLE MULTIPLICITY[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RapidityMultiplicity (chemistry)Nuclear Experiment010306 general physicsDELPHIPhysicsAnnihilation010308 nuclear & particles physicsLARGE ELECTRON POSITRON COLLIDERPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSHigh Energy Physics::ExperimentFRAGMENTATIONParticle Physics - Experiment
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Multiplicity fluctuations in one- And two-dimensional angular intervals compared with analytic QCD calculations

1999

Multiplicity fluctuations in rings around the jet axis and in off-axis cones have been measured by the DELPHI collaboration in $e^+e^-$ annihilations into hadrons at LEP energies. The measurements are compared with analytical perturbative QCD calculations for the corresponding multiparton system, using the concept of Local Parton Hadron Duality. Some qualitative features are confirmed by the data but substantial quantitative deviations are observed.

Nuclear and High Energy PhysicsParticle physicsHadronFOS: Physical sciencesParton01 natural sciencesPartícules (Física nuclear)HADRON SPECTRAHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesCOHERENCE[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Multiplicity (chemistry)010306 general physicsNuclear ExperimentParticle Physics - PhenomenologyDELPHIPhysicsQuantum chromodynamics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPerturbative QCDLARGE ELECTRON POSITRON COLLIDERHigh Energy Physics - PhenomenologyHADRON SPECTRA; MULTIPARTON CORRELATIONS; PERTURBATIVE-QCD; PARTON JETS; COHERENCE; INTERMITTENCYPARTON JETSPERTURBATIVE-QCDPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIINTERMITTENCYPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentMULTIPARTON CORRELATIONS
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