Search results for "física nuclear"

showing 10 items of 900 documents

High resolution 80Se(n,γ) cross section measurement at CERN n_TOF and development of the novel i-TED detection system

2022

El proceso (-s) de captura lenta de neutrones es responsable de la formación de la mitad de los elementos más pesados ​​que el hierro en el universo. A pesar de la larga escala de tiempo de este proceso, la larga vida media de algunos isótopos inestables a lo largo del flujo de reacción del proceso-s crea puntos de ramificación que conducen a una división de la ruta de la nucleosíntesis. 79Se (t1/2 = 3.27 x 10^5 y) representa uno de los núcleos ramificados-s más relevantes y debatidos por dos razones principales. Por un lado, la existencia de estados excitados de baja energía en el 79Se, cuya población puede variar con la temperatura del medio estelar, hace que el patrón de abundancia local…

Dynamic Electronic Collimationbranching pointPETsys Electronicsnucleosynthesisi-TEDprompt-gammaUNESCO::FÍSICA::Física atómica y nuclear ::Física nuclear experimental bajas energíasneutron capture cross sectionnuclear physics79Se:FÍSICA::Física atómica y nuclear ::Física nuclear experimental bajas energías [UNESCO]time of flightmonolithic scintillation crystalMACStotal energy detectorsbackground rejectionsilicon photomultipliers-processCompton camera80Se
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Gluon mass generation in the presence of dynamical quarks

2013

We study in detail the impact of dynamical quarks on the gluon mass generation mechanism, in the Landau gauge, for the case of a small number of quark families. As in earlier considerations, we assume that the main bulk of the unquenching corrections to the gluon propagator originates from the fully dressed quark-loop diagram. The nonperturbative evaluation of this diagram provides the key relation that expresses the unquenched gluon propagator as a deviation from its quenched counterpart. This relation is subsequently coupled to the integral equation that controls the momentum evolution of the effective gluon mass, which contains a single adjustable parameter; this constitutes a major impr…

Dyson-schwinger equationsQuarkHigh Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::LatticeNuclear TheoryBackground field methodFOS: Physical sciencesPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeGluon fieldPhysicsBackground field methodMass generationHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyPropagatorGluonMass formulaHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Gluon field strength tensorQuantum electrodynamicsHigh Energy Physics::Experiment
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WCxf: An exchange format for Wilson coefficients beyond the Standard Model

2018

We define a data exchange format for numerical values of Wilson coefficients of local operators parameterising low-energy effects of physics beyond the Standard Model. The format facilitates interfacing model-specific Wilson coefficient calculators, renormalisation group (RG) runners, and observable calculators. It is designed to be unambiguous (defining a non-redundant set of operators with fixed normalisation in each basis), extensible (allowing the addition of new EFTs or bases by the user), and robust (being based on industry standard file formats with parsers implemented in many programming languages). We have implemented the format for the Standard Model EFT (SMEFT) and for the weak e…

EFTSParsing010308 nuclear & particles physicsComputer scienceProgramming languagePhysics beyond the Standard ModelFOS: Physical sciencesGeneral Physics and AstronomyPython (programming language)computer.software_genreFile format01 natural sciencesPartícules (Física nuclear)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Hardware and ArchitectureData exchangeInterfacing0103 physical sciencesElectroweak scale010306 general physicscomputercomputer.programming_language
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Measurement of lifetimes in Fe-62,Fe-64, Co-61,Co-63, and Mn-59

2017

Lifetimes of the 4(1)(+) states in Fe-62,Fe-64 and the 11/2(1)(-) states in Co-61,Co-63 and Mn-59 were measured at the Grand Accelerateur National d'Ions Lourds (GANIL) facility by using the Advanced Gamma Tracking Array (AGATA) and the large-acceptance variable mode spectrometer (VAMOS++). The states were populated through multinucleon transfer reactions with a U-238 beam impinging on a Ni-64 target, and lifetimes in the picosecond range were measured by using the recoil distance Doppler shift method. The data show an increase of collectivity in the iron isotopes approaching N = 40. The reduction of the subshell gap between the nu 2p(1/2) and nu 1g(9/2) orbitals leads to an increased popul…

Electromagnetisme MesuramentsFísica nuclear
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D-0-(D-0)over-bar mixing in the weak-gauged U(4)(L)circle times U(4)(R) chiral Lagrangian model

1998

The D-0- mixing is analyzed in a weak gauged U(4)(L) x U(4)(R) chiral lagrangian model where the electroweak interaction is introduced as a gauge theory over the meson degrees of freedom. This model allows a particular realization of the G.I.M. mechanism and then could be useful in the study of processes where G.I.M. suppression is effective. As a test of the model we have also analyzed the K-0- mixing. We find am, in good agreement with the experimental result and we show that the D-0- mixing is very much suppressed in agreement with previous estimates in the Heavy Quark expansion framework.

Electromagnetisme MesuramentsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentFísica nuclear
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Description and commissioning of NEXT-MM prototype: first results from operation in a Xenon-Trimethylamine gas mixture

2014

[EN] A technical description of NEXT-MM and its commissioning and first performance is reported. Having an active volume of ∼35 cm drift × 28 cm diameter, it constitutes the largest Micromegas-read TPC operated in Xenon ever constructed, made by a sectorial arrangement of the 4 largest single wafers manufactured with the Microbulk technique to date. It is equipped with a suitably pixelized readout and with a sufficiently large sensitive volume (∼23 l) so as to contain long (∼20 cm) electron tracks. First results obtained at 1 bar for Xenon and Trymethylamine (Xe-(2%)TMA) mixture are presented. The TPC can accurately reconstruct extended background tracks. An encouraging fu…

Enginyeria -- InstrumentsMECANICA DE LOS MEDIOS CONTINUOS Y TEORIA DE ESTRUCTURASMaterials sciencePhysics - Instrumentation and DetectorsTime projection chambersParticle tracking detectors (Gaseous detectors)chemistry.chemical_elementTrimethylamineFOS: Physical sciencesElectron7. Clean energyEngineering instrumentsTECNOLOGIA ELECTRONICAchemistry.chemical_compoundXenonOpticsWafer[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]InstrumentationMathematical PhysicsDetectors de radiacióTime projection chamberbusiness.industryActive volumeMicroMegas detectorInstrumentation and Detectors (physics.ins-det)Double-beta decay detectorschemistryVolume (thermodynamics)Nuclear countersFísica nuclearbusiness
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Isospin mixing and in-beam study of non-yrast states in Co-56

2018

En el presente trabajo hemos estudiado la reacción de fusión-evaporación 56Fe(p,n gamma)56Co con un haz incidente de protones de 10 MeV en el Maier-Leibnitz-Laboratory (MLL) de la Technische Universität München (TUM, Alemania). Los rayos gamma emitidos en la desexcitación del núcleo impar-impar 56Co fueron medidos "in-beam" con cuatro detectores triples de germanio de alta resolución MINIBALL. El experimento proveyó excelentes datos en las coincidencias gamma-gamma. Un total de 223 transiciones gamma han sido observadas y colocadas en el esquema de niveles del 56Co, de las cuales 169 son gammas observadas por primera vez. Un total de 77 estados excitados han sido observador: 37 de ellos era…

Estructura nuclear:FÍSICA::Electromagnetismo ::Rayos gamma [UNESCO]:FÍSICA::Física atómica y nuclear ::Estructura nuclear [UNESCO]Análisis de datosUNESCO::MATEMÁTICAS::Estadística ::Análisis de datosShell model:MATEMÁTICAS::Estadística ::Análisis de datos [UNESCO]UNESCO::FÍSICA::Física atómica y nuclear ::Física nuclear experimental bajas energíasUNESCO::FÍSICA::Electromagnetismo ::Rayos gammaEspectroscopía gamma:FÍSICA::Física atómica y nuclear ::Física nuclear experimental bajas energías [UNESCO]Physics::Atomic and Molecular ClustersUNESCO::FÍSICA::Física atómica y nuclear ::Estructura nuclearFísica nuclear experimental
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B-0-(B)over-bar(0) mixing and decay constants with the non-perturbatively improved action

2001

Several quantities relevant to phenomenological studies of B-0-(B) over bar (0) mixing are computed on the lattice. Our main results are f(Bd) root(B) over cap (Bd) = 206(28) (14)(-00)(+31) MeV, xi = f(Bd) root(B) over capB(x)/f(Bd) root(B) over cap (Bd) = 1.16(7). We also obtain the related quantities f(Bs) root(B) over cap (Bs) - 237(18) (10)(-00)(+34) MeV, f(Bd) = 174(22)(-0-0-00)(+7+5+26) MeV, f(Bs) = 204(15)(-0-0-00)(+7+4+31) MeV, f(Bs)/f(Bd) = 1.17(4)(-1)(+0), f(Bd)/f(Ds) = 0.74(5). After combining our results with the experimental world average Deltam(d)((exp)), we predict Deltam(s) = 15.8(2.1)(3.3) ps(-1). We have also computed the relevant parameters for D-0-(D) over bar (0) mixing…

FIS/02 - FISICA TEORICA MODELLI E METODI MATEMATICIB physics gauge theory latticePartícules (Física nuclear)
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Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory

2012

The energy spectrum of ultra-high energy cosmic rays above 10$^{18}$ eV is measured using the hybrid events collected by the Pierre Auger Observatory between November 2005 and September 2010. The large exposure of the Observatory allows the measurement of the main features of the energy spectrum with high statistics. Full Monte Carlo simulations of the extensive air showers (based on the CORSIKA code) and of the hybrid detector response are adopted here as an independent cross check of the standard analysis (Phys. Lett. B 685, 239 (2010)). The dependence on mass composition and other systematic uncertainties are discussed in detail and, in the full Monte Carlo approach, a region of confiden…

FLUORESCENCE DETECTORAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesCosmic RayAugerPierre Auger Observatory ; Monte Carlo simulations ; ultra-high energy cosmic raysHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesRECONSTRUCTIONFermilab010306 general physicsUHE Cosmic Rays Monte Carlo Energy SpectrumTRIGGERNuclear PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryPACS: 96.50.S 96.50.sb 96.50.sd 98.70.Sa010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger Observatory; Monte Carlo simulations; ultra-high energy cosmic raysPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryPROFILES[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]Experimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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Search for ultrarelativistic magnetic monopoles with the Pierre Auger Observatory

2016

We present a search for ultra-relativistic magnetic monopoles with the Pierre Auger Observatory. Such particles, possibly a relic of phase transitions in the early universe, would deposit a large amount of energy along their path through the atmosphere, comparable to that of ultrahigh-energy cosmic rays (UHECRs). The air shower profile of a magnetic monopole can be effectively distinguished by the fluorescence detector from that of standard UHECRs. No candidate was found in the data collected between 2004 and 2012, with an expected background of less than 0.1 event from UHECRs. The corresponding 90% confidence level (C.L.) upper limits on the flux of ultra-relativistic magnetic monopoles ra…

FLUORESCENCE YIELDAstronomymagnetic monopolemagnetic fieldAstrophysics7. Clean energy01 natural sciencesObservatoryUHE Cosmic Raysair-showerMonte Carlo010303 astronomy & astrophysicsMagnetic Monopolesmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicscritical phenomenaFLUORESCENCE YIELD; ENERGY LOSS; DETECTORAugerMagnetic fieldobservatoryLorentz factorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical Phenomenaspatial distribution [showers]LorentzENERGY LOSSatmosphere [showers]energyFLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]airmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]Magnetic monopoleFOS: Physical sciencesCosmic rayNuclear physicssymbols.namesakecosmic rays0103 physical sciencesddc:530High Energy PhysicsDETECTORCiencias Exactasfluorescence [detector]Pierre Auger Observatorybackground010308 nuclear & particles physicsFísicaASTROFÍSICAUniversefluxultrarelativistic magnetic monopolesAir shower13. Climate actionExperimental High Energy PhysicsrelativisticgalaxyENERGY-LOSS
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