Search results for "ENERGIES"

showing 10 items of 168 documents

Nuclear data activities at the n_TOF facility at CERN

2016

International audience; Nuclear data in general, and neutron-induced reaction cross sections in particular, are important for a wide variety of research fields. They play a key role in the safety and criticality assessment of nuclear technology, not only for existing power reactors but also for radiation dosimetry, medical applications, the transmutation of nuclear waste, accelerator-driven systems, fuel cycle investigations and future reactor systems as in Generation IV. Applications of nuclear data are also related to research fields as the study of nuclear level densities and stellar nucleosynthesis. Simulations and calculations of nuclear technology applications largely rely on evaluate…

Nuclear reactionU-235Nuclear transmutationnTOFCAPTURE CROSS-SECTIONNuclear dataTOTAL ABSORPTION CALORIMETERGeneral Physics and Astronomy[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]COLLABORATION7. Clean energy01 natural sciences3100PHYSICSNuclear physicsPhysics and Astronomy (all)neutronDESIGNRadiation dosimetry0103 physical sciencesCERNn_TOFNuclear Physics - ExperimentNeutron010306 general physicsnuclear data n_TOF CERNPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsFRAGMENT ANGULAR-DISTRIBUTIONLarge Hadron Colliderntof:Física [Àrees temàtiques de la UPC]Cross section010308 nuclear & particles physicscernExperimental dataRadioactive wasteNuclear datanuclear dataNATURAL SCIENCES. Physics.Radiació--DosimetriaPRIRODNE ZNANOSTI. Fizika.Nuclear technologyCAPTURE CROSS-SECTION TOTAL ABSORPTION CALORIMETER FRAGMENT ANGULAR-DISTRIBUTION NEUTRON TH-232 U-235 C6D6 COLLABORATION PHYSICS DESIGN.NEUTRONTH-232C6D6
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The 33S(n,α)30Si cross section measurement at n TOF-EAR2 (CERN): From 0.01 eV to the resonance region

2017

The 33S(n,α)30Si cross section measurement, using 10B(n,α) as reference, at the n TOF Experimental Area 2 (EAR2) facility at CERN is presented. Data from 0.01 eV to 100 keV are provided and, for the first time, the cross section is measured in the range from 0.01 eV to 10 keV. These data may be used for a future evaluation of the cross section because present evaluations exhibit large discrepancies. The 33S(n,α)30Si reaction is of interest in medical physics because of its possible use as a cooperative target to boron in Neutron Capture Therapy (NCT).

Nuclear reactionnTOFNeutron therapyQC1-999chemistry.chemical_elementNeutron01 natural sciencesResonance (particle physics)Nuclear physicsCross section (physics)Physics and Astronomy (all)0103 physical sciencesCERNNeutronddc:530010306 general physicsBoronPhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]Range (particle radiation)Large Hadron Collidercross sectionReaccions nuclears:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear reactionNeutron capturechemistryNuclear reactions
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High precision measurement of the radiative capture cross section of 238U at the n_TOF CERN facility

2016

The importance of improving the accuracy on the capture cross-section of 238U has been addressed by the Nuclear Energy Agency, since its uncertainty significantly affects the uncertainties of key design parameters for both fast and thermal nuclear reactors. Within the 7th framework programme ANDES of the European Commission three different measurements have been carried out with the aim of providing the 238U(n,γ) cross-section with an accuracy which varies from 1 to 5%, depending on the energy range. Hereby the final results of the measurement performed at the n-TOF CERN facility in a wide energy range from 1 eV to 700 keV will be presented. © The Authors, published by EDP Sciences, 2017.

Nuclear reactionnTOFQC1-999Neutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsCross section (physics)Physics and Astronomy (all)Nuclear reactorsReactors nuclears0103 physical sciencesThermalCERNNeutronddc:530Nuclear Physics - Experiment010306 general physicsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsRange (particle radiation)Large Hadron Collider:Física [Àrees temàtiques de la UPC]Cross section010308 nuclear & particles physicsPhysicsRadiative captureNuclear energyNuclear reactionEnergia nuclearEnergy (signal processing)
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The 236U neutron capture cross-section measured at the n TOF CERN facility

2016

International audience; The $^{236}$U isotope plays an important role in nuclear systems, both for future and currently operating ones. The actual knowledge of the capture reaction of this isotope is satisfactory in the thermal region, but it is considered insufficient for Fast Reactor and ADS applications. For this reason the $^{236} \text{U}(n, \gamma)$ reaction cross-section has been measured for the first time in the whole energy region from thermal energy up to 1 MeV at the n_TOF facility with two different detection systems: an array of C$_6$D$_6$ detectors, employing the total energy deposited method, and a 4$\pi$ total absorption calorimeter (TAC), made of 40 BaF$_2$ crystals. The t…

Nuclear reactionnTOFQC1-999Neutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Cross section (physics)0103 physical sciencesCERNNeutron cross sectionNuclear Physics - Experimentddc:530Neutron010306 general physicsAbsorption (electromagnetic radiation)PhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]IsotopeCross sectionReaccions nuclears:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsResonanceNuclear reactionCalorimeter13. Climate actionNuclear reactions
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New measurement of the 242Pu(n,γ) cross section at n-TOF-EAR1 for MOX fuels: Preliminary results in the RRR

2016

The spent fuel of current nuclear reactors contains fissile plutonium isotopes that can be combined with 238U to make mixed oxide (MOX) fuel. In this way the Pu from spent fuel is used in a new reactor cycle, contributing to the long-term sustainability of nuclear energy. The use of MOX fuels in thermal and fast reactors requires accurate capture and fission cross sections. For the particular case of 242Pu, the previous neutron capture cross section measurements were made in the 70’s, providing an uncertainty of about 35% in the keV region. In this context, the Nuclear Energy Agency recommends in its “High Priority Request List” and its report WPEC-26 that the capture cross section of 242Pu…

Nuclear reactionnTOFQC1-999Nuclear engineeringContext (language use)CERN nTOFNeutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyPhysics and Astronomy (all)Nuclear reactorsReactors nuclears0103 physical sciencesCERNNeutron cross sectionNuclear Physics - ExperimentNeutronddc:530242Pu neutron capture010306 general physicsMOX fuelNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]Fissile materialCross section:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear reactionSpent nuclear fuelNeutron temperature13. Climate actionneutron time-of-flight measurement
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The ANTARES telescope neutrino alert system

2012

The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

Optical telescopesPhysics::Instrumentation and DetectorsAstrophysics7. Clean energy01 natural sciencesGamma ray burstsFOLLOW-UP OBSERVATIONSlaw.inventionlawFlaring activeVery high energiesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGAMMA-RAY BURSTS[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsSupernovaNeutrino detectorNeutrino astronomyFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesOptical telescopeTelescopeMuon tracksCoincidentSEARCHDetection methods0103 physical sciencesCore collapse supernovae010306 general physicsOptical follow-upInstrumentation and Methods for Astrophysics (astro-ph.IM)Neutronsantares; neutrino astronomy; optical follow-up; transient sourcesANTARES010308 nuclear & particles physicsGamma raysAstronomyAstronomy and AstrophysicsAlert systemsStarsTransient sources[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Optical signalsPotential sources13. Climate actionFISICA APLICADAHigh Energy Physics::ExperimentNeutrino astronomyGamma-ray burst
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Energy Management Systems and tertiary regulation in hierarchical control architectures for islanded microgrids

2015

In this paper, the structure of the highest level of a hierarchical control architecture for micro-grids is proposed. Such structure includes two sub-levels: the Energy Management System, EMS, and the tertiary regulation. The first devoted to energy resources allocation in each time slot based on marginal production costs, the latter aiming at finding the match between production and consumption satisfying the constraints set by the EMS level about the energy production in each time slot. Neglecting the efficiency of the different energy generation systems as well as that of the infrastructure for electrical energy distribution, the problem dealt with by the EMS sub-level is linear and can …

OptimizationEngineeringMathematical optimizationMicro-gridsLinear programmingEnergy managementbusiness.industry:Energies [Àrees temàtiques de la UPC]Electric potential energyControl engineeringElectric powerEnergy management systemSettore ING-IND/33 - Sistemi Elettrici Per L'EnergiaElectricity generationEnergy management systemsLinear programmingEnergia elèctricaElectric powerMinificationbusinessInteger programmingEnergy management systems linear programming microgrids optimization
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Event-by-event fluctuations in a perturbative QCD plus saturation plus hydrodynamics model : Determining QCD matter shear viscosity in ultrarelativis…

2016

We introduce an event-by-event perturbative-QCD + saturation + hydro ("EKRT") framework for ultrarelativistic heavy-ion collisions, where we compute the produced fluctuating QCD-matter energy densities from next-to-leading-order perturbative QCD using a saturation conjecture to control soft-particle production and describe the space-time evolution of the QCD matter with dissipative fluid dynamics, event by event. We perform a simultaneous comparison of the centrality dependence of hadronic multiplicities, transverse momentum spectra, and flow coefficients of the azimuth-angle asymmetries against the LHC and RHIC measurements. We compare also the computed event-by-event probability distribut…

PB-PB COLLISIONSMULTIPLICITIES01 natural sciences114 Physical sciencesGLUON DISTRIBUTION-FUNCTIONSquantum chromodynamicshydrodynamics model0103 physical sciencesFluid dynamics010306 general physicsNuclear ExperimentTRANSVERSE ENERGIESKINETIC-THEORYQCD matterPhysicsta114010308 nuclear & particles physicsDISSIPATIVE FLUID-DYNAMICSELLIPTIC FLOWShear viscosityElliptic flowHigh Energy Physics::PhenomenologyPerturbative QCDheavy-ion collisionsCENTRALITY DEPENDENCEFREEZE-OUTShear (geology)Quantum electrodynamicsRELATIVISTIC NUCLEAR COLLISIONSQuark–gluon plasmaDissipative system
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Parc fotovoltaic de la Universitat de València

2009

Energies alternatives. Parc fotovoltaic de la Universitat de València.

Parc Fotovoltaic Energies renovables Plaques solars Parc Científic
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Search for pair production of heavy objects in 4-jet events at sqrt {s}$=130-136 GeV

1996

Results are presented of a search for pair production of heavy objects decaying into four hadronic jets, as expected for example from associated or pair production of MSSM Higgs bosons, hA or H$^+$H$^-$, using a data sample of $5.9\,$pb$^{-1}$ of $e^+ e^-$ collisions at $\sqrt{s}=130$-$136\,{\mathrm {GeV}}$ collected with the DELPHI detector at LEP in November 1995. The data and expectations from standard processes agree after four-jet selections. An analysis based on $b$-tagging finds no hA candidate with high mass. A study optimized to search for H$^+$H$^-$ events with mass in the 40-50$\,{\mathrm{GeV}}/c^2$ range also finds no candidate. Finally a comparison is made with a recent ALEPH a…

Particle physicsAlephPhysics and Astronomy (miscellaneous)ENERGIESElectron–positron annihilationHadronHIGGS BOSONSJet (particle physics)Partícules (Física nuclear)DECAYSNuclear physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors de radiacióBosonDELPHIPhysicsHigh Energy Physics::PhenomenologySupersymmetryLARGE ELECTRON POSITRON COLLIDERHIGGS BOSONS; ENERGIES; DECAYSPair productionPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIHiggs bosonPARTICLE PHYSICSHigh Energy Physics::ExperimentParticle Physics - Experiment
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