Search results for "SPECTRA"

showing 10 items of 3542 documents

Time resolved photoluminescence associated with non-bridging oxygen hole centers in irradiated silica

2008

Abstract We report time resolved photoluminescence spectra of irradiated silica under excitation with a laser tunable in the visible and UV range. The investigated samples exhibit the emission band at 1.9 eV associated with non-bridging oxygen hole centers, whose spectral and kinetics properties do not depend on the kind of irradiation (γ, β and neutrons). The 1.9 eV luminescence decay follows a multi-exponential curve with a characteristic lifetime that increases from 8.9 μs to 10.4 μs on increasing the emission energy. This dependence accounts for the blue-shift of the emission band during its decay and is interpreted as due to the inhomogeneous properties of silica leading to a distribut…

Nuclear and High Energy PhysicsRange (particle radiation)PhotoluminescenceMaterials scienceKineticsAnalytical chemistryDefects Silica Radiation effectsLaserMolecular physicsSpectral linelaw.inventionlawAstrophysics::Earth and Planetary AstrophysicsIrradiationLuminescenceInstrumentationExcitationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Optimization of a conversion electron Mössbauer spectroscopy gas flow He/CH4 proportional counter

1992

A new detector for CEMS has been built and optimized with respect to the statistical quality of spectra obtained. The optimization has been performed by measuring Mosbauer and pulse height spectra at in- and off-resonance. Single channel analyzer settings were calculated by a new optimization routine. A comparison of different detector designs has been performed using the statistical utility rate of spectra obtained from a stainless steel foil. A procedure for determining optimal operating parameters for ICEMS gas flow proportional counters is proposed.

Nuclear and High Energy PhysicsSpectrum analyzerMaterials sciencePhysics::Instrumentation and DetectorsDetectorFlow (psychology)Analytical chemistryProportional counterCondensed Matter PhysicsAtomic and Molecular Physics and OpticsSpectral lineConversion electron mössbauer spectroscopyPhysical and Theoretical ChemistryFOIL methodPulse heightHyperfine Interactions
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Dark radiation and interacting scenarios

2013

An extra dark radiation component can be present in the universe in the form of sterile neutrinos, axions or other very light degrees of freedom which may interact with the dark matter sector. We derive here the cosmological constraints on the dark radiation abundance, on its effective velocity and on its viscosity parameter from current data in dark radiation-dark matter coupled models. The cosmological bounds on the number of extra dark radiation species do not change significantly when considering interacting schemes. We also find that the constraints on the dark radiation effective velocity are degraded by an order of magnitude while the errors on the viscosity parameter are a factor of…

Nuclear and High Energy PhysicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterCosmological parametersCosmic background radiationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesCosmologyRadiacióPower spectrumsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010303 astronomy & astrophysicsAxionTelescopeDigital sky surveyPhysicsCosmologiaHubble constant010308 nuclear & particles physicsSpectral densityMicrowave background anisotropiesHigh Energy Physics - Phenomenology13. Climate actionDark radiationConstraintssymbolsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Sterile neutrinos or flux uncertainties? — Status of the reactor anti-neutrino anomaly

2017

The $\sim 3\sigma$ discrepancy between the predicted and observed reactor anti-neutrino flux, known as the reactor anti-neutrino anomaly, continues to intrigue. The recent discovery of an unexpected bump in the reactor anti-neutrino spectrum, as well as indications that the flux deficit is different for different fission isotopes seems to disfavour the explanation of the anomaly in terms of sterile neutrino oscillations. We critically review this conclusion in view of all available data on electron (anti)neutrino disappearance. We find that the sterile neutrino hypothesis cannot be rejected based on global data and is only mildly disfavored compared to an individual rescaling of neutrino fl…

Nuclear and High Energy PhysicsSterile neutrinoFissionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesElectron01 natural sciencesSpectral lineHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Flux (metallurgy)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530010306 general physicsPhysicsIsotope010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentAnomaly (physics)NeutrinoJournal of High Energy Physics
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Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos

2018

We discuss the possibility to explain the anomalies in short-baseline neutrino oscillation experiments in terms of sterile neutrinos. We work in a 3+1 framework and pay special attention to recent new data from reactor experiments, IceCube and MINOS+. We find that results from the DANSS and NEOS reactor experiments support the sterile neutrino explanation of the reactor anomaly, based on an analysis that relies solely on the relative comparison of measured reactor spectra. Global data from the $\nu_e$ disappearance channel favour sterile neutrino oscillations at the $3\sigma$ level with $\Delta m^2_{41} \approx 1.3$ eV$^2$ and $|U_{e4}| \approx 0.1$, even without any assumptions on predicte…

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsFOS: Physical sciences01 natural sciences7. Clean energySpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNeutrino Physicslcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530010306 general physicsNeutrino oscillationMixing (physics)Particle Physics - PhenomenologyPhysicshep-ex010308 nuclear & particles physicsOscillationPhysicsHigh Energy Physics::Phenomenologyhep-ph3. Good healthHigh Energy Physics - PhenomenologyMINOSBeyond Standard Modellcsh:QC770-798High Energy Physics::ExperimentAnomaly (physics)NeutrinoParticle Physics - ExperimentJournal of High Energy Physics
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Confirmation of gA quenching using the revised spectrum-shape method for the analysis of the 113Cd β-decay as measured with the COBRA demonstrator

2021

In this article we present an updated spectrum-shape analysis of the $^{113}$Cd fourfold forbidden non-unique $\beta$-decay transition in order to address the quenching of the weak axial-vector coupling $g_{\rm A}$ in low-momentum exchange nuclear processes. The experimental data were collected in a dedicated low-threshold run with the COBRA demonstrator at the LNGS and resulted in 44 individual $^{113}$Cd spectra. These data are evaluated in the context of three nuclear model frameworks based on a revised version of the spectrum-shape method and the conserved vector current hypothesis. The novel idea devised in the present work is to fit the value of the small relativistic nuclear matrix e…

Nuclear and High Energy PhysicsWork (thermodynamics)Nuclear Theoryspectrum-shape methodQC1-999Value (computer science)Context (language use)gA quenchingSpectrum-shape method01 natural sciencesSpectral lineNuclear physicsaxial-vector coupling113Cd β-decayAxial-vector coupling0103 physical sciences010306 general physicsNuclear ExperimentCOBRACouplingPhysicsQuenching010308 nuclear & particles physicsPhysicsNuclear structureCdZnTeydinfysiikkaFree parameterPhysics Letters B
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Transverse momentum spectra and nuclear modification factors of charged particles in Xe–Xe collisions at √sNN = 5.44 TeV

2019

Transverse momentum (pT) spectra of charged particles at mid-pseudorapidity in Xe–Xe collisions at √sNN = 5.44 TeV measured with the ALICE apparatus at the Large Hadron Collider are reported. The kinematic range 0.15 10 GeV/c. The centrality dependence of the ratio of the average transverse momentum (pT) in Xe–Xe collisions over Pb–Pb collision at √s = 5.02 TeV is compared to hydrodynamical model calculations. peerReviewed

Nuclear and High Energy PhysicsXe–Xe collisionstransverse momentum spectraHigh Energy Physics::ExperimenthiukkasfysiikkaNuclear Experiment
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Two-dimensional single- and multiple-quantum correlation spectroscopy in zero-field nuclear magnetic resonance.

2020

We present single- and multiple-quantum correlation $J$-spectroscopy detected in zero ($<\!\!1$~$\mu$G) magnetic field using a \Rb vapor-cell magnetometer. At zero field the spectrum of ethanol appears as a mixture of \carbon isotopomers, and correlation spectroscopy is useful in separating the two composite spectra. We also identify and observe the zero-field equivalent of a double-quantum transition in ${}^{13}$C$_2$-acetic acid, and show that such transitions are of use in spectral assignment. Two-dimensional spectroscopy further improves the high resolution attained in zero-field NMR since selection rules on the coherence-transfer pathways allow for the separation of otherwise overlappi…

Nuclear and High Energy PhysicsZero field NMRMagnetometerNuclear Magnetic Resonancephysics.chem-phBiophysicsFOS: Physical sciences010402 general chemistry01 natural sciencesBiochemistryMolecular physicsSpectral line030218 nuclear medicine & medical imagingIsotopomerslaw.invention03 medical and health sciences0302 clinical medicineEngineeringquant-phlawPhysics - Chemical PhysicsJ-Spectroscopy2D NMRSpectroscopyPhysicsChemical Physics (physics.chem-ph)Quantum PhysicsCorrelation spectroscopyZero (complex analysis)Zero-field NMRCondensed Matter PhysicsMultiple-quantum NMR3. Good health0104 chemical sciencesMagnetic fieldZULF NMRPhysical SciencesQuantum Physics (quant-ph)Two-dimensional nuclear magnetic resonance spectroscopy
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Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is describe…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumFluxFOS: Physical sciencesCosmic rayAstrophysicsElectronSURFACE DETECTORUPPER LIMITENERGIAPHOTON FRACTION01 natural sciencesSpectral lineAugerNuclear physicscosmic raysObservatorySHOWERS0103 physical sciencesHigh-Energy Cosmic Ray010306 general physicsCosmic raysCiencias ExactasPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Spectral densityFísicaPierre Auger ObservatoryCosmic rayELECTRONS3. Good healthPierre Auger Observatory; Cosmic rays; Energy spectrumSIMULATIONExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaARRAYFísica nuclearEnergy spectrumAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Properties of nuclei in the nobelium region studied within the covariant, Skyrme, and Gogny energy density functionals

2015

We calculate properties of the ground and excited states of nuclei in the nobelium region for proton and neutron numbers of 92 &lt;= Z &lt;= 104 and 144 &lt;= N &lt;= 156, respectively. We use three different energy-density-functional (EDF) approaches, based on covariant, Skyrme, and Gogny functionals, each within two different parameter sets. A comparative analysis of the results obtained for odd-even mass staggerings, quasiparticle spectra, and moments of inertia allows us to identify single-particle and shell effects that are characteristic to these different models and to illustrate possible systematic uncertainties related to using the EDF modelling

Nuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]ProtonNuclear TheoryNuclear Theorychemistry.chemical_elementFOS: Physical sciences7. Clean energySpectral lineMoments of inertiaNuclear physicsNuclear Theory (nucl-th)NeutronCovariant transformationHeavy and superheavy nucleiPhysicsta114Odd–even mass staggeringMoment of inertiachemistryExcited stateQuasiparticleNobeliumQuasiparticle excitationsNuclear energy density functionalsNuclear masses
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