Search results for "LIMIT"

showing 10 items of 2826 documents

Technical challenges in the construction of the steady-state stellarator Wendelstein 7-X

2013

The next step in the Wendelstein stellarator line is the large superconducting device Wendelstein 7-X, currently under construction in Greifswald, Germany. Steady-state operation is an intrinsic feature of stellarators, and one key element of the Wendelstein 7-X mission is to demonstrate steady-state operation under plasma conditions relevant for a fusion power plant. Steady-state operation of a fusion device, on the one hand, requires the implementation of special technologies, giving rise to technical challenges during the design, fabrication and assembly of such a device. On the other hand, also the physics development of steady-state operation at high plasma performance poses a challeng…

Nuclear and High Energy PhysicsSteady state (electronics)LIMIT ANALYSISPLASMANuclear engineeringMAGNET SYSTEMPlasmaFusion powerCondensed Matter PhysicsW7-XElectron cyclotron resonancelaw.inventionPHYSICSData acquisitionHeating systemlawWendelstein 7-XStellarator
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Solar and Atmospheric Four-Neutrino Oscillations

2001

We present an analysis of the neutrino oscillation solutions of the solar and atmospheric neutrino problems in the framework of four-neutrino mixing where a sterile neutrino is added to the three standard ones and the mass spectra presents two separated doublets. Such scenarios allow for simultaneous transitions of solar $\nu_e$, as well as atmospheric $\nu_\mu$, into active and sterile neutrinos controlled by the additional mixing angles $\vartheta_{23}$ and $\vartheta_{24}$, and they contain as limiting cases the pure solar $\nu_e$-active and $\nu_e$-sterile neutrino oscillations, and the pure atmospheric $\nu_\mu\to\nu_s$ and $\nu_\mu\to\nu_\tau$ oscillations, respectively. We evaluate t…

Nuclear and High Energy PhysicsSterile neutrinoAstrofísica nuclearOscillationsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)BibliographyOscil·lacionsAstrophysics::Solar and Stellar AstrophysicsNeutrinsNeutrinosNeutrino oscillationMixing (physics)Particle Physics - PhenomenologyParticles (Nuclear physics)PhysicsHigh Energy Physics::PhenomenologyLimitingHigh Energy Physics - PhenomenologyAstronomiaMass spectrumNuclear astrophysicsHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsAtmospheric neutrino
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Strangeness-changing scalar form factors

2001

30 páginas, 2 tablas, 10 figuras.-- arXiv:hep-ph/0110193v1

Nuclear and High Energy PhysicsStrange quarkParticle physicsNuclear TheoryScalar form factorsHadronScalar (mathematics)FOS: Physical sciencesStrangenessMeson–meson interactionsResonance (particle physics)High Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)Coupled channelsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeLimit (mathematics)PhysicsQCD sum rulesHigh Energy Physics - Lattice (hep-lat)Momentum transferFísicaFinal state interactionsHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentChiral lagrangians
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Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is describe…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumFluxFOS: Physical sciencesCosmic rayAstrophysicsElectronSURFACE DETECTORUPPER LIMITENERGIAPHOTON FRACTION01 natural sciencesSpectral lineAugerNuclear physicscosmic raysObservatorySHOWERS0103 physical sciencesHigh-Energy Cosmic Ray010306 general physicsCosmic raysCiencias ExactasPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Spectral densityFísicaPierre Auger ObservatoryCosmic rayELECTRONS3. Good healthPierre Auger Observatory; Cosmic rays; Energy spectrumSIMULATIONExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaARRAYFísica nuclearEnergy spectrumAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Measuring the isotope effect on the gross beryllium erosion in JET

2022

Abstract The isotope effect, hydrogen (H) versus deuterium (D), on the gross beryllium (Be) erosion yield has been measured in ohmic limiter plasmas in JET tokamak by spectroscopic means. A simplified method to extract the effective sputtering yield from the quotient of the radiances of the D α or D γ and the Be II lines at 527 nm was applied. A clear isotope effect has been found, the erosion yield of D being about a factor of 2 larger compared to H in the whole explored plasma density range. This is in agreement with physical sputtering data obtained with H+ and D+ ion beams and also with material surface computer simulations. The already published contribution of chemically assisted phys…

Nuclear and High Energy PhysicsspectroscopyJETsputteringddc:620Condensed Matter Physicsberylliumerosionisotopelimiter
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An upper limit for the τ neutrino mass from τ → 5π(π0)ντ decays

1995

An upper limit for the tau-neutrino mass has been determined from the decay tau -> 5pi+- \nu_tau using data collected with the OPAL detector from 1991 to 1995 in e+e- collisions at \sqrt{s} ~ M_Z. A limit of 43.2 MeV at 95% CL is obtained using a two-dimensional method in the 5pi invariant mass and energy distribution from 22 selected events. Combining this result with OPAL's previously published measurement using tau+tau- -> 3h+- \bar{nu}_tau 3h-+ \nu_tau decays, a new combined limit of m_{nu_tau} < 27.6 MeV (95% CL) is obtained.

Nuclear physicsPhysicsALEPH ExperimentNuclear and High Energy PhysicsParticle physicsEnergy distributionElectron–positron annihilationPhysicsHigh Energy Physics::ExperimentInvariant massLimit (mathematics)NeutrinoBar (unit)
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Improved limit on the electron-antineutrino rest mass from tritium ß-decay

1993

Abstract The endpoint region of the β-spectrum of tritium was remeasured by an electrostatic spectrometer with magnetic guiding field. It enabled the search for a rest mass of the electron-antineutrino with improved precision. The result is m2v=−39±34stat±15syst(eV/c2)2, from which an upper limit of mv m( T )−m( 3 He )=18 591±3 eV /c 2 .

Nuclear physicsPhysicsNuclear and High Energy PhysicsField (physics)SpectrometerElectron energy spectrumTritiumInvariant massddc:530Limit (mathematics)Atomic physicsElectron neutrino
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Limit on νe→ντ oscillations from the NOMAD experiment

2000

Abstract In the context of a two-flavour approximation we reinterpret the published NOMAD limit on ν μ → ν τ oscillations in terms of ν e → ν τ oscillations. At 90% C.L. we obtain sin 2 2θ eτ 5.2×10 −2 for large Δm 2 , while for sin 2 2 θ eτ =1 the confidence region includes Δm 2 2 / c 4 .

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physics0103 physical sciencesContext (language use)Limit (mathematics)Neutrino beam010306 general physicsNeutrino oscillation01 natural sciencesCharged currentPhysics Letters B
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Search for the decay KS → π0γγ

2003

Abstract A search for the decay K S → π 0 γγ has been made using the NA48 detector at the CERN SPS. Using data collected in 1999 during a 40-hour run with a high-intensity K S beam, an upper limit for the branching ratio BR ( K S → π 0 γγ , z ⩾0.2) −7 has been obtained at 90% confidence level, where z = m γγ 2 / m K 0 2 .

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsBranching fraction0103 physical sciencesDetectorLimit (mathematics)010306 general physics01 natural sciencesBeam (structure)
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Measurement of the mass and width of the charmed meson D∗+ (2010)

1992

Abstract Using a high-resolution silicon vertex detector we have observed a very clean signal of 127 D∗+. After a careful study of the experimental resolution of our apparatus we have measured m( D ∗++ )−m( D 0 ) = 145.39±0.06±0.03 MeV . We have also obtained a 90% CL upper limit to γ(D∗+) of 131 keV.

Nuclear physicsPhysicsNuclear and High Energy PhysicsParticle physicsMesonPhysics::Instrumentation and DetectorsResolution (electron density)High Energy Physics::ExperimentLimit (mathematics)SignalParticle Physics - ExperimentSilicon vertex detectorPhysics Letters B
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