Search results for "Energia nuclear"

showing 10 items of 28 documents

Measurement of the a ratio and (n,¿) cross section of U 235 from 0.2 to 200 eV at n_TOF

2020

We measured the neutron capture-to-fission cross-section ratio (a ratio) and the capture cross section of 235U between 0.2 and 200 eV at the n_TOF facility at CERN. The simultaneous measurement of neutron-induced capture and fission rates was performed by means of the n_TOF BaF2 Total Absorption Calorimeter (TAC), used for detection of ¿ rays, in combination with a set of micromegas detectors used as fission tagging detectors. The energy dependence of the capture cross section was obtained with help of the 6 Li(n,t) standard reaction determining the n_TOF neutron fluence; the well-known integral of the 235U(n, f ) cross section between 7.8 and 11 eV was then used for its absolute normalizat…

:Energies::Energia nuclear [Àrees temàtiques de la UPC]:Física [Àrees temàtiques de la UPC]Nuclear physicsNuclear fissionFísica nuclearNeutrons--CapturaNeutrons--CaptureFissió nuclear
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Measurement and analysis of the 241-Am neutron capture cross section at the n_TOF facility at CERN

2018

The 241Am(n,¿ ) cross section has been measured at the n_TOF facility at CERN with the n_TOF BaF2 Total Absorption Calorimeter in the energy range between 0.2 eV and 10 keV. Our results are analyzed as resolved resonances up to 700 eV, allowing a more detailed description of the cross section than in the current evaluations, which contain resolved resonances only up to 150–160 eV. The cross section in the unresolved resonance region is perfectly consistent with the predictions based on the average resonance parameters deduced from the resolved resonances, thus obtaining a consistent description of the cross section in the full neutron energy range under study. Below 20 eV, our results are i…

:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsNuclear engineering:Física [Àrees temàtiques de la UPC]Cross sectionnTOFEnginyeria nuclearCERNNuclear physicsFísica nuclearNeutronNuclear reaction
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Beta Decay Studies of Neutron Rich Nuclei Using Total Absorption Gamma-ray Spectroscopy and Delayed Neutron Measurements

2010

International audience; A complete characterisation of the β-decay of neutron-rich nuclei can be obtained from the measurement of β-delayed gamma rays and, whenever the process is energetically possible, β-delayed neutrons. The accurate determination of the β-intensity distribution and the β-delayed neutron emission probability is of great relevance in the fields of reactor technology and nuclear astrophysics. A programme for combined measurements using the total absorption gamma-ray spectroscopy technique and both neutron counters and neutron time-of-flight spectrometers is presented.

Astrofísica nuclearNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryGeneral Physics and AstronomyBeta decayNeutron scattering[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesNuclear physicsPrompt neutronNuclear Technology0103 physical sciencesNuclear AstrophysicsNeutron cross sectionNeutronDelayed neutrons emission010306 general physicsNuclear ExperimentSpectroscopyPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Total Absorption Gamma-Rayta114010308 nuclear & particles physicsRadioactivitat betaNeutron stimulated emission computed tomographyBeta DecayDelayed Neutron Emission3. Good healthNeutron Detectors23.40.Bw 29.30.KvNuclear astrophysicsPrompt neutronsDelayed neutronNeutron activation
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The BRIKEN Project: Extensive Measurements of $\beta $-delayed Neutron Emitters for the Astrophysical r Process

2018

An ambitious program to measure decay properties, primarily β-delayed neutron emission probabilities and half-lives, for a significant number of nuclei near or on the path of the rapid neutron capture process, has been launched at the RIKEN Nishina Center. We give here an overview of the status of the project.

AstrofísicaDelayed neutronNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear dataNuclear TheoryMeasure (physics)General Physics and AstronomyNeutronAstrophysics01 natural sciencesNuclear physics0103 physical sciencesNeutronNuclear Experiment010306 general physics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPhysics:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNuclear dataNeutron capture:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]r-processDelayed neutronActa Physica Polonica B
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Commissioning of the BRIKEN beta-delayed neutron detector for the study of exotic neutron-rich nuclei

2017

Beta-delayed neutron emission (Beta-n) is a form of radioactive decay in which an electron, an anti-neutrino and one or more neutrons are emitted. This process arises if the energy window of the decay Q_Beta is greater than the neutron separation energy S n of the daughter. The probability in each decay of emitting neutrons is called the Pn value. This form of decay plays a key role in the synthesis of chemical elements in the Universe via the rapid neutron capture process, or r-process. The r-process proceeds far from the valley of nuclear stability, and leads to very neutron-rich nuclei that then decay to the line of stability. Most of these nuclei are ßn emitters. The initial abundance d…

AstrofísicaNeutron emissionQC1-999Astrophysics::High Energy Astrophysical PhenomenaNeutron detectorNuclear TheoryElectronNeutronAstrophysics01 natural sciencesNuclear physics0103 physical sciencesNeutron detectionNeutron010306 general physicsNuclear ExperimentDelayed neutronsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Neutrons:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear structureDetectorNeutron captureDelayed neutronRadioactive decay
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7Be(n,α) and 7Be(n,p) cross-section measurement for the cosmological lithium problem at the n-TOF facility at CERN

2017

One of the most puzzling problems in Nuclear Astrophysics is the “Cosmological Lithium Problem”, i.e the discrepancy between the primordial abundance of \(^{7}\)Li observed in metal poor halo stars (Asplund et al. in Astrophys J 644:229–259, 2006, [1]), and the one predicted by Big Bang Nucleosynthesis (BBN). One of the reactions that could have an impact on the problem is \(^{7}\)Be(n,p)\(^{7}\)Li. Despite of the importance of this reaction in BBN, the cross-section has never been directly measured at the energies of interest for BBN. Taking advantage of the innovative features of the second experimental area at the n\(\_\)TOF facility at CERN (Sabate-Gilarte et al. in Eur Phys J A 53:210,…

AstrofísicanTOFQC1-999chemistry.chemical_elementNeutronAstrophysics01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Big Bang nucleosynthesisNucleosynthesisCERN0103 physical sciencesNuclear astrophysicsAstrophysics::Solar and Stellar AstrophysicsNeutron010306 general physicsNuclear ExperimentAstrophysics::Galaxy Astrophysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPhysicsAlphaLarge Hadron Collider:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsStarschemistryLithiumHaloNucleosynthesisNucleosíntesi
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The n_TOF facility: Neutron beams for challenging future measurements at CERN

2016

The CERN n TOF neutron beam facility is characterized by a very high instantaneous neutron flux, excellent TOF resolution at the 185 m long flight path (EAR-1), low intrinsic background and coverage of a wide range of neutron energies, from thermal to a few GeV. These characteristics provide a unique possibility to perform high-accuracy measurements of neutron-induced reaction cross-sections and angular distributions of interest for fundamental and applied Nuclear Physics. Since 2001, the n TOF Collaboration has collected a wealth of high quality nuclear data relevant for nuclear astrophysics, nuclear reactor technology, nuclear medicine, etc. The overall efficiency of the experimental prog…

AstrofísicanTOF[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]QC1-999Nuclear TheoryNeutronAstrophysics01 natural sciences7. Clean energylaw.inventionNuclear physicsPhysics and Astronomy (all)Neutron fluxlaw0103 physical sciencesCERNNuclear astrophysicsNeutronSpallation010306 general physicsNuclear ExperimentPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsLarge Hadron Collider:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear dataNuclear reactorNeutron radiationAccelerators and Storage Rings3. Good health13. Climate action
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¿Es la energía nuclear la solución al cambio climático? Editorial

2004

El 24 de mayo 2004 el periódico inglés The Independent publicó un artículo de James Lovelock, el conocido autor de la Hipótesis Gaia , con el título Nuclear power is the only green solution ( La energía nuclear es la única solución verde ) que tuvo una notable repercusión en los medios de comunicación, en los que se llegó a afirmar que el propio Mikhail Gorbatxov, Presidente de Green Cross International, apoyaba estas tesis favorables al uso de la energía nuclear.

Canvi mediambiental globalEnergia nuclear
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Electroluminescence TPCs at the thermal diffusion limit

2019

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

ElectroluminiscènciaNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsDark Matter and Double Beta DecayFOS: Physical scienceschemistry.chemical_elementElectronAtomic01 natural sciences7. Clean energyMathematical SciencesHigh Energy Physics - ExperimentTECNOLOGIA ELECTRONICAHigh Energy Physics - Experiment (hep-ex)Particle and Plasma PhysicsXenonIonization0103 physical sciencesDark Matter and Double Beta Decay (experiments)Nuclearlcsh:Nuclear and particle physics. Atomic energy. RadioactivityDiffusion (business)010306 general physicsMathematical PhysicsPhysicsQuantum Physics010308 nuclear & particles physicsResolution (electron density)MolecularFísicaNuclear energyInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsParticle correlations and fluctuations85-05ElectroluminescencechemistryRare decayYield (chemistry)Photon productionPhysical SciencesScintillation counterEnergia nuclearlcsh:QC770-798Atomic physicsEnergy (signal processing)
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Near-intrinsic energy resolution for 30-662 keV gamma rays in a high pressure xenon electroluminescent TPC

2013

We present the design, data and results from the NEXT prototype for Double Beta and Dark Matter (NEXT-DBDM) detector, a high-pressure gaseous natural xenon electroluminescent time projection chamber (TPC) that was built at the Lawrence Berkeley National Laboratory. It is a prototype of the planned NEXT-100 Xe-136 neutrino-less double beta decay (0 nu beta beta) experiment with the main objectives of demonstrating near-intrinsic energy resolution at energies up to 662 keV and of optimizing the NEXT-100 detector design and operating parameters. Energy resolutions of similar to 1% FWHM for 662 keV gamma rays were obtained at 10 and 15 atm and similar to 5% FWHM for 30 keV fluorescence xenon X-…

ElectroluminiscènciaNuclear and High Energy PhysicsXenonHigh-pressureDark matterchemistry.chemical_elementNuclear physicsTECNOLOGIA ELECTRONICAXenonDouble beta decayEnergy resolutionNeutrinoless double beta decayInstrumentationPhysicsTime projection chamberDetectorResolution (electron density)Gamma rayFísicaNuclear energyFull width at half maximumchemistryElectroluminescenceEnergia nuclearTPC
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