Search results for "nuclear physics"

showing 10 items of 5307 documents

Muons in air showers at the Pierre Auger Observatory

2015

We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously with the surface detector array and the fluorescence detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019eV shower with a zenith angle of 67°, which arrives at the surface detector array at an altitude of 1450 m above sea level, contains on average (2.68±0.04±0.48(sys))×107 muons with energies large…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCosmic-ray interactionsAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayextensive atmospherical showers muon density muon number Pierre Auger Observatory cosmic radiation UHEHadronic interaction models7. Clean energyAugerSettore FIS/04 - Fisica Nucleare e SubnucleareNuclear physicsAltitudeSettore FIS/05 - Astronomia e AstrofisicaObservatoryNERGY COSMIC-RAYS DETECTOR MODEL.Extensive air showerscosmic radiation UHEDETECTORScalingCosmic raysZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryMuonNERGY COSMIC-RAYSSettore FIS/01 - Fisica Sperimentaleenergy cosmic-rays; detector; modelAstrophysics::Instrumentation and Methods for AstrophysicsFísica[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ObservatoryASTROFÍSICAextensive atmospherical showersmuon numberMODELmuon densityExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaPhysical Review D
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Physics at a future Neutrino Factory and super-beam facility

2009

The conclusions of the Physics Working Group of the international scoping study of a future Neutrino Factory and super-beam facility (the ISS) are presented. The ISS was carried by the international community between NuFact05, (the 7th International Workshop on Neutrino Factories and Superbeams, Laboratori Nazionali di Frascati, Rome, June 21-26, 2005) and NuFact06 (Ivine, California, 24{30 August 2006). The physics case for an extensive experimental programme to understand the properties of the neutrino is presented and the role of high-precision measurements of neutrino oscillations within this programme is discussed in detail. The performance of second generation super-beam experiments, …

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsPhysics::Instrumentation and DetectorsMUONIUM-ANTIMUONIUM CONVERSIONFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2LONG-BASE-LINE01 natural sciences7. Clean energyWARM DARK-MATTERNuclear physicsLEPTON-FLAVOR VIOLATIONELECTRIC-DIPOLE MOMENTHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ANOMALOUS MAGNETIC-MOMENT010306 general physicsNeutrino oscillationNeutrino physics; Neutrino factoryParticle Physics - PhenomenologyR-PARITY VIOLATIONPhysicsMuonAnomalous magnetic dipole moment010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]LARGE EXTRA DIMENSIONSDOUBLE-BETA-DECAYNeutrino factoryFísicaMU-E CONVERSIONNeutrino physicsHigh Energy Physics - PhenomenologyExperimental High Energy PhysicsLarge extra dimensionCP violationPhysics::Accelerator PhysicsNeutrino FactoryHigh Energy Physics::ExperimentNeutrino
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Upper limit on the cosmic-ray photon fraction at EeV energies from the Pierre Auger Observatory

2009

From direct observations of the longitudinal development of ultra-high energy air showers performed with the Pierre Auger Observatory, upper limits of 3.8%, 2.4%, 3.5% and 11.7% (at 95% c.l.) are obtained on the fraction of cosmic-ray photons above 2, 3, 5 and 10 EeV (1 EeV equivalent to 10(18) eV), respectively. These are the first experimental limits on ultra-high energy photons at energies below 10 EeV. The results complement previous constraints on top-down models from array data and they reduce systematic uncertainties in the interpretation of shower data in terms of primary flux, nuclear composition and proton-air cross-section.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhotonAstronomyFOS: Physical sciencesFluxCosmic rayFotonesAstrophysicsEXTENSIVE AIR-SHOWERS01 natural sciences7. Clean energyNuclear physicsCascada atmosféricaUltra high energy (UHE)0103 physical sciencesLimit (mathematics)FLUORESCENCEUltra-high energy cosmic ray010303 astronomy & astrophysicsDETECTORCosmic raysCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysics010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FísicaAstronomy and AstrophysicsPierre Auger ObservatoryPROFILESRadiación cósmicaPhotonLongitudinal development13. Climate actionphoton fractionComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical Phenomena
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The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory

2011

In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the probability for an Extensive Air Shower (EAS) to trigger an individual detector of a ground based array as a function of distance to the shower axis, taking into account energy, mass and direction of the primary cosmic ray. We apply this concept to the surface array of the Pierre Auger Observatory consisting of a 1.5 km spaced grid of about 1600 water Cherenkov stations. Using Monte Carlo simulations of ultra-high energy showers the LTP functions are derived for energies in the range between 1017 and 1019 eV and zenith angles up to 65. A parametrization combining a step function with an exponenti…

[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]AstronomyAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerUltra-high Energy Cosmic RayMonte Carlo methodFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSTrigger performance01 natural sciences7. Clean energyUltra-high Energy Cosmic Rays; Pierre Auger Observatory; Extensive air showers; Trigger performance; Surface detector; Hybrid detectorHigh Energy Physics - ExperimentAugerNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsCiencias ExactasZenithCherenkov radiationUltra-High Energy Cosmic RaysPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysicsHybrid detector[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Surface detectorAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high Energy Cosmic Rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearExtensive Air ShowersAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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"Safe" Coulomb excitation of 30Mg.

2004

We report on the first radioactive beam experiment performed at the recently commissioned REX-ISOLDE facility at CERN in conjunction with the highly efficient $\gamma$ -spectrometer MINIBALL. Using $^{30}$Mg ions accelerated to an energy of 2.25MeV/u together with a thin $^{nat}$Ni target, Coulomb excitation of the first excited 2+ states of the projectile and target nuclei well below the Coulomb barrier was observed. From the measured relative de-excitation $\gamma$ -ray yields the B(E2; 0$^{+}_{gs} \rightarrow 2^{+}_{1}$) value of $^{30}$Mg was determined to be 241(31)$e^{2}$fm$^{4}$. Our result is lower than values obtained at projectile fragmenttion facilities using the intermediate-ene…

[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]Coulomb excitationFOS: Physical sciencesPhysics::Accelerator PhysicsNuclear Physics - Experiment25.70.De 27.30.+t 21.10.ReNuclear Experiment (nucl-ex)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear ExperimentCollective levels20 < A < 38Radioactive beamsPhysical review letters
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Identification of new transitions feeding the high-spin isomers in $^{139}$Nd and $^{140}$Nd nuclei

2013

The population of the high-spin isomers in 139Nd and 140Nd was investigated using the 96Zr(48Ca,xn) reaction and the JUROGAM + RITU + GREAT setup employing the recoil decay tagging technique. Three transitions feeding the 23/2+ isomer in 139Nd and two transitions feeding the 20+ isomer in 140Nd were identified. The newly observed transitions allowed the excitation energy of the isomer to be established in 139Nd and to assign configurations to the states and bands deexcited by the observed transitions in both nuclei. peerReviewed

[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]ComputingMilieux_MISCELLANEOUSExperimental Nuclear Physics
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Isotope Shifts of Radium Monofluoride Molecules

2021

Isotope shifts of $^{223-226,228}$Ra$^{19}$F were measured for different vibrational levels in the electronic transition $A^{2}{}{\Pi}_{1/2}\leftarrow X^{2}{}{\Sigma}^{+}$. The observed isotope shifts demonstrate the particularly high sensitivity of radium monofluoride to nuclear size effects, offering a stringent test of models describing the electronic density within the radium nucleus. Ab initio quantum chemical calculations are in excellent agreement with experimental observations. These results highlight some of the unique opportunities that short-lived molecules could offer in nuclear structure and in fundamental symmetry studies.

[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th]FIELD SHIFTNuclear TheoryAtomic Physics (physics.atom-ph)Ab initioGeneral Physics and AstronomyNUCLEAR-STRUCTUREnucl-ex01 natural sciencesPhysics - Atomic Physics010305 fluids & plasmasENERGYchemistry.chemical_compoundatomifysiikkaMOMENTSPhysics::Atomic PhysicsNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentPhysicsIsotopePhysicsNuclear structureradiumNuclear Physics - TheoryPhysical SciencesAtomic physicsydinfysiikkanucl-th[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Monofluoride[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex][PHYS.PHYS.PHYS-GEN-PH] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Physics MultidisciplinaryOther Fields of PhysicsFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]physics.atom-phMolecular electronic transitionELECTRONIC-STRUCTURE CALCULATIONSNuclear Theory (nucl-th)ATOMS0103 physical sciencesMoleculeSPECTRANuclear Physics - ExperimentSensitivity (control systems)010306 general physicsisotoopitScience & Technology[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]chemistryMECHANICSMASS DEPENDENCELASERElectronic density
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A sum rule approach to total muon capture rates

1986

Abstract The total muon capture rate is expanded in terms of sum rules and the convergence of such an expansion is analyzed. It results that the energy-weighted and the inverse-energy-weighted sum rules provide an accurate estimate for the total rate in agreement with a complete RPA calculation through the response function. The static polarizability of the isovector dipole mode turns out to be the relevant quantity to determine the total muon capture rate, in light and medium nuclei.

[PHYS.NUCL] Physics [physics]/Nuclear Theory [nucl-th]PhysicsNuclear and High Energy PhysicsIsovector[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]010308 nuclear & particles physicsNuclear TheoryFunction (mathematics)01 natural sciencesMuon captureNuclear physicsDipole modePolarizability0103 physical sciencesConvergence (routing)Rule of sumSum rule in quantum mechanicsAtomic physics010306 general physics
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Charge radius of the short-lived $^{68}$Ni and correlation with the dipole polarizability

2020

We present the first laser spectroscopic measurement of the neutron-rich nucleus $^{68}$Ni at the \mbox{$N=40$} subshell closure and extract its nuclear charge radius. Since this is the only short-lived isotope for which the dipole polarizability $\alpha_{\rm D}$ has been measured, the combination of these observables provides a benchmark for nuclear structure theory. We compare them to novel coupled-cluster calculations based on different chiral two- and three-nucleon interactions, for which a strong correlation between the charge radius and dipole polarizability is observed, similar to the stable nucleus $^{48}$Ca. Three-particle--three-hole correlations in coupled-cluster theory substant…

[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear Theorynucl-thNuclear TheoryFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-exNuclear Theory (nucl-th)Nuclear Physics - Theoryddc:530Nuclear Physics - ExperimentPhysics::Atomic PhysicsNuclear Experiment (nucl-ex)Präzisionsexperimente - Abteilung BlaumNuclear ExperimentNuclear ExperimentNuclear Physics
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Prospects for advanced electron cyclotron resonance and electron beam ion source charge breeding methods for EURISOL

2011

International audience; As the most ambitious concept of isotope separation on line (ISOL) facility, EURISOL aims at producing unprecedented intensities of post-accelerated radioactive isotopes. Charge breeding, which transforms the charge state of radioactive beams from 1+ to an n+ charge state prior to postacceleration, is a key technology which has to overcome the following challenges: high charge states for high energies, efficiency, rapidity and purity. On the roadmap to EURISOL, a dedicated R&D is being undertaken to push forward the frontiers of the present state-of-the-art techniques which use either electron cyclotron resonance or electron beam ion sources. We describe here the gui…

[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Cyclotron resonanceplasmafysiikka01 natural sciences7. Clean energyElectron cyclotron resonanceIonlaw.inventionIsotope separationelectron beamsNuclear physicsEURISOLion sourceslaw0103 physical sciencescyclotron resonance010306 general physicsradioactive ion beamsradioactive beamInstrumentation010302 applied physicsPhysicsta11429.25.Ni 41.75.Fr 07.77.KaionilähteetParticle acceleratorradioaktiiviset suihkutIon sourceCathode rayAtomic physicsydinfysiikkaIon cyclotron resonance
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