Search results for "Física de Partículas"

showing 10 items of 50 documents

Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

2011

We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 × 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.

Large scale anisotripies[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Auger ExperimentAstronomyAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesCosmic rayAstrophysicsanisotropySURFACE DETECTOR01 natural sciencesCosmic RayAugerLarge scale anisotropiesObservatoryLarge scale anisotropie0103 physical sciences010303 astronomy & astrophysicsUltra-high energy cosmic rayCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryFÍSICA DE PARTÍCULASUltra High Energy Cosmic Rays.010308 nuclear & particles physicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high energy cosmic raysENERGY-SPECTRUMRadiación cósmicaAnisotropíaAmplitudeHarmonicsUltra-high energy cosmic rays; Large scale anisotropies; Pierre Auger ObservatoryExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearRight ascensionAstrophysics - High Energy Astrophysical Phenomena
researchProduct

On the nature of Dark Matter: phenomenological and cosmological probes

2018

La evidencia gravitatoria de la materia oscura es incuestionable. Sin embargo, la naturaleza de la materia oscura representa uno de los mayores enigmas de la Física moderna. Gracias a las precisas observaciones del fondo cósmico de microondas realizadas por los satélites WMAP y Planck sabemos que un ~26% del contenido energético del universo y que un ~84% de toda la materia corresponde a un tipo de materia que solo interactúa gravitatoriamente. Además, multitud de estudios demuestran que las galaxias, cúmulos de galaxias, así como de la mayoría de objetos virializados en el universo están dominados por una materia que no emite luz, la materia oscura. La indiscutible evidencia gravitatoria d…

Materia OscuraCosmologíaFísica de Partículas
researchProduct

Coherent neutrino scattering

2009

We present a microscopic model for coherent pion production off nuclei induced by neutrinos. This model is built upon a model for single nucleon processes that goes beyond the usual Delta dominance by including non resonant background contributions. We include nuclear medium effects: medium corrections to Delta$ properties and outgoing pion absortion via an optical potential. This results in major modifications to cross sections for low energy experiments when compared with phenomenological models like Rein-Sehgal's.

Modelo microscópico ; Producción de piones ; Rein–Sehgal’sRein–Sehgal’sNuclear TheoryAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryUNESCO::FÍSICAUNESCO::FÍSICA::Nucleónica::Física de partículasFOS: Physical sciencesProducción de pionesNuclear Theory (nucl-th):FÍSICA [UNESCO]:FÍSICA::Nucleónica::Física de partículas [UNESCO]Nuclear ExperimentModelo microscópicoPhysics::Atmospheric and Oceanic Physics
researchProduct

Lifetime measurements of excited states in neutron-rich nuclei around 48 Ca

2009

The lifetimes of the first excited states of the N = 30 isotones 50Ca and 51Sc and the Z = 18 isotopes 44−46Ar isotopes have been determined using a novel technique that combines the Recoil Distance Doppler Shift method with the CLARA-PRISMA spectrometers in multinucleon transfer reactions. The results allow determinination of the effective charges above 48Ca and test the strength of the N = 28 magic number when moving away from the stability line. Gadea Raga, Andrés, Gadea.Andres@ific.uv.es ; Algora, Alejandro, Alejandro.Algora@ific.uv.es ; Rubio Barroso, Berta, Berta.Rubio@ific.uv.es

Multinucleon transfer reactionMultinucleon transfer reaction ; Isotopes ; Recoil Distance Doppler Shift ; CLARA-PRISMAIsotopes:FÍSICA [UNESCO]:FÍSICA::Nucleónica::Física de partículas [UNESCO]UNESCO::FÍSICAUNESCO::FÍSICA::Nucleónica::Física de partículasCLARA-PRISMARecoil Distance Doppler Shift
researchProduct

β-Delayed and isomer spectroscopy of neutron-rich Ta and W isotopes

2009

Decays of neutron-rich A ~ 190 nuclei have been studied following projectile fragmentation of a 208Pb beam on a 9Be target at the GSI Fragment Separator. Gamma-ray decays from previously reported isomeric states in 188Ta, 190W and 192, 193Re were used as internal calibrations for the particle identification analysis, together with the identification of previously unreported isomeric decays in 189Ta and 191W. The current work also identifies β-delayed γ rays following the decay of 188Ta to 188W for the first time. Algora, Alejandro, Alejandro.Algora@ific.uv.es ; Molina Palacios, Francisco Manuel, Francisco.Molina@ific.uv.es; Rubio Barroso, Berta, Berta.Rubio@ific.uv.es

Neutron-rich ; Projectile fragmentation ; GSI Fragment Separator ;:FÍSICA [UNESCO]:FÍSICA::Nucleónica::Física de partículas [UNESCO]UNESCO::FÍSICAUNESCO::FÍSICA::Nucleónica::Física de partículasNeutron-richGSI Fragment SeparatorProjectile fragmentation
researchProduct

βDelayed γRay spectroscopy of heavy neutron rich nuclei “south” of lead

2009

Relativistic projectile fragmentation of a 208Pb primary beam has been used to produce neutron-rich nuclei with proton-holes relative to the Z = 82 shell closure, i.e., “south” of Pb. βDelayed γRay spectroscopy allows to investigate the structural properties of such nuclei with A ~ 195 → 205. The current work presents transitions de-exciting excited states in 204Au, which are the first spectroscopic information on this N = 125 isotone. Agramunt Ros, Jorge, Jorge.Agramunt@ific.uv.es ; Algora, Alejandro, Alejandro.Algora@ific.uv.es ; Molina Palacios, Francisco Manuel, Francisco.Molina@ific.uv.es ; Rubio Barroso, Berta, Berta.Rubio@ific.uv.es

Neutron-rich nuclei:FÍSICA [UNESCO]:FÍSICA::Nucleónica::Física de partículas [UNESCO]Relative projectile fragmentationUNESCO::FÍSICAUNESCO::FÍSICA::Nucleónica::Física de partículasProton-holesRelative projectile fragmentation ; Neutron-rich nuclei ; Proton-holes ; SpectroscopySpectroscopy
researchProduct

Population of neutron-rich nuclei around 48ca with deep inelastic collisions

2009

The deep inelastic reaction 48Ca+64Ni at 6 MeV/A has been studied using the CLARA–PRISMA setup. Angular distributions for pure elastic scattering and total cross-sections of the most relevant transfer channels have been measured. The experimental results are compared with predictions from a semiclassical model, showing good agreement for the presently analyzed few neutrons transfer channels. The decay of the most intense reaction products has also been studied, giving indications of the population of states with very short lifetimes. Gadea Raga, Andrés, Gadea.Andres@ific.uv.es

Neutron-rich nucleiReacción InelásticaUNESCO::FÍSICAUNESCO::FÍSICA::Nucleónica::Física de partículasInelastic collision Neutron-rich nuclei Reaction products Semiclassical model Transfer channel; Angular distribution; CalciumReaction productsCanales de transmisiónSemiclassical modelCLARA–PRISMAReacción Inelástica ; CLARA–PRISMA ; Distribuciones angulares ; Secciones cruzadas ; Modelo semiclásico ; Canales de transmisión ; Muy corta vidaInelastic collisionDistribuciones angularesdeep inelastic reaction; semiclassical model; closed shell nuceli:FÍSICA [UNESCO]:FÍSICA::Nucleónica::Física de partículas [UNESCO]Muy corta vidaTransfer channelSecciones cruzadasCalciumAngular distributionModelo semiclásico
researchProduct

Third family of compact stars within a nonlocal chiral quark model equation of state

2019

A class of hybrid compact star equations of state is investigated that joins by a Maxwell construction a low-density phase of hadronic matter, modeled by a relativistic mean-field approach with excluded nucleon volume, with a high-density phase of color superconducting two-flavor quark matter, described within a nonlocal covariant chiral quark model. It is found that the occurrence of a stable branch of hybrid compact stars requires a nonvanishing vector meson coupling in the quark model that exceeds a minimal value which depends on the presence of a diquark condensate. It is shown that these hybrid stars do not form a third family disconnected from the second family of ordinary neutron sta…

Particle physicsEquation of stateNuclear TheoryCiencias FísicasNuclear TheoryFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsCompact starFísica de Partículas y Campos//purl.org/becyt/ford/1 [https]Nuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)compact starsAstrophysics::Solar and Stellar AstrophysicsVector mesonquark modelsAstrophysics::Galaxy AstrophysicsPhysicsMaxwell construction//purl.org/becyt/ford/1.3 [https]Coupling (probability)Neutron starStarsStrange matterHigh Energy Physics - Phenomenologytwin starsAstrophysics::Earth and Planetary AstrophysicsCIENCIAS NATURALES Y EXACTAS
researchProduct

Collider aspects of flavour physics at high Q

2008

This chapter of the 'Flavor in the era of LHC' workshop report discusses flavor-related issues in the production and decays of heavy states at the LHC at high momentum transfer Q, both from the experimental and the theoretical perspective. We review top quark physics, and discuss the flavor aspects of several extensions of the standard model, such as supersymmetry, little Higgs models or models with extra dimensions. This includes discovery aspects, as well as the measurement of several properties of these heavy states. We also present publicly available computational tools related to this topic. © Springer-Verlag / Società Italiana di Fisica 2008.

Particle physicsTop quarkPhysics and Astronomy (miscellaneous)High Energy Physics::LatticeFlavourFOS: Physical sciences01 natural scienceslaw.inventionStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesddc:530High Energy Physics010306 general physicsColliderHadronesEngineering (miscellaneous)Flavour PhysicParticle Physics - PhenomenologyPhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaLittle HiggsSupersymmetryExtra dimensionsHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physique des particules élémentairesFísica de partículasHigh Energy Physics::ExperimentLHCColisionadoresCollider
researchProduct

Measurement of the inclusive jet cross-section in pp collisions at $\sqrt{s}=2.76\ \mbox{TeV}$ and comparison to the inclusive jet cross-section at $…

2013

The inclusive jet cross-section has been measured in proton-proton collisions at sqrt(s)=2.76 TeV in a dataset corresponding to an integrated luminosity of 0.20pb-1 collected with the ATLAS detector at the Large Hadron Collider in 2011. Jets are identified using the anti-kt algorithm with two radius parameters of 0.4 and 0.6. The inclusive jet double-differential cross-section is presented as a function of the jet transverse momentum pT and jet rapidity y, covering a range of 20 <= pT < 430 GeV and |y| < 4.4. The ratio of the cross-section to the inclusive jet cross-section measurement at sqrt(s)=7 TeV, published by the ATLAS Collaboration, is calculated as a function of both trans…

Physics and Astronomy (miscellaneous)Cern Pbarp ColliderCiencias FísicasMonte Carlo methodParton01 natural sciences7. Clean energyHigh Energy Physics - ExperimentEp Scattering//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)PhysicsLarge Hadron ColliderSettore FIS/01 - Fisica SperimentalePerturbative QCDATLASPerturbation-TheoryINCLUSIVE JET CROSS SECTIONPhysical SciencesLHCCIENCIAS NATURALES Y EXACTASParticle Physics - ExperimentParticle physicsShowersCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesFísica de Partículas y CamposNuclear physicsDeep-Inelastic ScatteringFragmentation0103 physical sciencesFysikRapidityddc:530High Energy Physics010306 general physicsEngineering (miscellaneous)Science & Technology010308 nuclear & particles physicsParton DistributionsFísica//purl.org/becyt/ford/1.3 [https]Deep inelastic scatteringDistribution function(P)over-Bar-P CollisionsHADRON-HADRON COLLISIONSExperimental High Energy PhysicsHigh Energy Physics::ExperimentDimensionless quantityModelThe European Physical Journal C
researchProduct