Search results for "Isòtops radioactius"

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Initial results of NEXT-DEMO, a large-scale prototype of the NEXT-100 experiment

2013

NEXT-DEMO is a large-scale prototype of the NEXT-100 detector, an electroluminescent time projection chamber that will search for the neutrinoless double beta decay of Xe-136 using 100-150 kg of enriched xenon gas. NEXT-DEMO was built to prove the expected performance of NEXT-100, namely, energy resolution better than 1% FWHM at 2.5MeV and event topological reconstruction. In this paper we describe the prototype and its initial results. A resolution of 1.75% FWHM at 511 keV (which extrapolates to 0.8% FWHM at 2.5 MeV) was obtained at 10 bar pressure using a gamma-ray calibration source. Also, a basic study of the event topology along the longitudinal coordinate is presented, proving that it…

MECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASPhysics - Instrumentation and DetectorsBar (music)Isòtops radioactius -- DesintegracióTime projection chambersPattern recognition SystemsFOS: Physical scienceschemistry.chemical_elementElectron7. Clean energy01 natural sciencesNuclear physicsTECNOLOGIA ELECTRONICAXenonCambres d'ionitzacióCluster analysisDouble beta decayPattern recognition0103 physical sciencesCalibrationReconeixement de formes (Informàtica)Calibratge010306 general physicsInstrumentationMathematical PhysicsRadioisotopes -- DecayPhysicsCalibration and fitting methodsTime projection chamber010308 nuclear & particles physicsDetectorCluster findingFísicaInstrumentation and Detectors (physics.ins-det)Double-beta decay detectorsAnàlisi de conglomeratschemistryCalibrationEvent (particle physics)Ionization Chambers
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Progress on nuclear reaction rates affecting the stellar production of 26Al

2023

Abstract The radioisotope 26Al is a key observable for nucleosynthesis in the Galaxy and the environment of the early Solar System. To properly interpret the large variety of astronomical and meteoritic data, it is crucial to understand both the nuclear reactions involved in the production of 26Al in the relevant stellar sites and the physics of such sites. These range from the winds of low- and intermediate-mass asymptotic giant branch stars; to massive and very massive stars, both their Wolf–Rayet winds and their final core-collapse supernovae (CCSN); and the ejecta from novae, the explosions that occur on the surface of a white dwarf accreting material from a stellar companion. Several r…

RadioisotopesRadioisotopeisotoopitNuclear and High Energy PhysicsIsòtops radioactiuscore-collapse supernovae (CCSN)tähdet:Física [Àrees temàtiques de la UPC]astrofysiikkaReaccions nuclears--TarifesnucleosynthesisNuclear reactions--Ratesnuclear reaction rateNuclear reaction rateydinreaktiotkääpiötähdetsupernovatradioisotope 26AlradioisotopealumiiniWolf-Rayet (WR) windsydinfysiikkaNucleosynthesisNucleosíntesi
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