Search results for "Neutro"

showing 10 items of 2997 documents

The Hamburg/ESO R-process Enhanced Star survey (HERES)

2004

We report on a dedicated effort to identify and study metal-poor stars strongly enhanced in r-process elements ([r/Fe] > 1 dex; hereafter r-II stars), the Hamburg/ESO R-process Enhanced Star survey (HERES). Moderate-resolution (~2A) follow-up spectroscopy has been obtained for metal-poor giant candidates selected from the Hamburg/ESO objective-prism survey (HES) as well as the HK survey to identify sharp-lined stars with [Fe/H] < -2.5dex. For several hundred confirmed metal-poor giants brighter than B~16.5mag (most of them from the HES), ``snapshot'' spectra (R~20,000; S/N~30 per pixel) are being obtained with VLT/UVES, with the main aim of finding the 2-3% r-II stars expected to be a…

population II [stars]PhysicsAstrophysics (astro-ph)FOS: Physical sciencesabundances [Galaxy]Astronomy and AstrophysicsAstrophysicsStar (graph theory)AstrophysicsSpectral lineabundances [stars]Neutron captureStarssurveysSpace and Planetary SciencePhenomenological modelhalo [Galaxy]Astronomy Astrophysics and Cosmologyr-processSpectroscopyRadioactive decayAstronomy & Astrophysics
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Sub-diffusive dynamics in hydrated myoglobin powder?

2008

protein dynamicneutron scattering
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The contribution of methyl groups dynamics to the dynamical transition of proteins

2008

protein dynamicneutron scatteringpolyaminoacids
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Neutroniaktivaatio puun kosteuden mittauksessa

2009

Kyseessä oli alustava tutkimus, jossa selvitettiin, onko neutroniaktivaation avulla mahdollista mitata puun kosteutta. Tarkasteltavana menetelmänä oli välittömien neutroniaktivaatiogammojen mittaaminen (PGNAA). Menetelmällä voidaan mitata alkuaineiden isotooppien suhteellisia osuuksia näytteissä.

puukosteusmittausneutroniaktivaatio
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Water Dynamics in Biological Systems investigated using Neutron Scattering Techniques

Living systems can not survive in absence of the water environments which play a fundamental role in living functions. Thus in the scienti?c community many studies were and are addressed to characterize water and its dynamics properties in biological systems. However, a clear description of water in such systems has been not reached yet. In fact, the investigations performed with di?erent techniques - those based on Nuclear Magnetic Resonance or those based on Neutron Scattering - look at di?erent di?usive motions and interactions water-biomolecules, leading controversial results and hence generating many debates between scientists. In this thesis we support the idea that two water populati…

quasi-elastic neutron scattering intracellular water water structure and dynamics bovine brain tissues cellular systems sucrose solutionsSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)
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Rotational effects on the oscillation frequencies of newly born proto-neutron stars

2003

In this paper we study the effects of rotation on the frequencies of the quasi-normal modes of a proto-neutron star (PNS) born in a gravitational collapse during the first minute of life. Our analysis starts a few tenths of seconds after the PNS formation, when the stellar evolution can be described by a sequence of equilibrium configurations. We use the evolutionary models developed by Pons et al. (1999; 2001) that describe how a non rotating star cools down and contracts while neutrino diffusion and thermalization processes dominate the stellar dynamics. For assigned values of the evolution time, we set the star into slow rotation and integrate the equations of stellar perturbations in th…

relativityFOS: Physical sciencesmethods : numericalAstrophysicsAstrophysicsInstabilitystars : oscillationsmethods: numericalstars: neutronstars: rotationstars : rotationStellar dynamicsGravitational collapseAstrophysics::Solar and Stellar AstrophysicsTime domainStellar evolutionPhysicsgravitational waves; methods : numerical; methods: numerical; relativity; stars : neutron; stars : oscillations; stars : rotation; stars: neutron; stars: oscillations; stars: rotationAstrophysics (astro-ph)Astronomy and Astrophysicsstars : neutronNeutron stargravitational wavesSpace and Planetary ScienceFrequency domainstars: oscillationsAstrophysics::Earth and Planetary AstrophysicsNeutrinoMonthly Notices of the Royal Astronomical Society
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Dangerous Effects Induced on Power MOSFETs by Terrestrial Neutrons

2013

This paper investigates the effects that terrestrial neutrons can induce on power MOSFETs when they are biased during their normal working conditions especially in inverters for photovoltaic applications. After a brief review of power MOSFETs failure phenomena caused by neutron irradiation (with emphasis on so called “Single Event Effects” (SEE)), the results of an accelerated test performed with the Am-Be source at the University of Palermo are discussed.

reliabilitypower MOSFETaccelerated testSEBSettore ING-IND/20 - Misure E Strumentazione NucleariTerrestrial neutronAm-Be sourceSettore ING-INF/01 - ElettronicaSEESEGR
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97/37 Rb 60 : The Cornerstone of the Region of Deformation around A∼100

2015

Excited states of the neutron-rich nuclei 97,99Rb were populated for the first time using the multistep Coulomb excitation of radioactive beams. Comparisons of the results with particle-rotor model calculations provide clear identification for the ground-state rotational band of 97Rb as being built on the πg9/2 [431] 3/2+ Nilsson-model configuration. The ground-state excitation spectra of the Rb isotopes show a marked distinction between single-particle-like structures below N=60 and rotational bands above. The present study defines the limits of the deformed region around A∼100 and indicates that the deformation of 97Rb is essentially the same as that observed well inside the deformed regi…

rubidiumneutron-rich nucleiCoulomb excitation
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97/37 Rb 60 : The Cornerstone of the Region of Deformation around A∼100

2015

rubidiumta114neutron-rich nucleiCoulomb excitationPhysical Review Letters
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Beta-decay studies for applied and basic nuclear physics

2020

In this review we will present the results of recent beta-decay studies using the total absorption technique that cover topics of interest for applications, nuclear structure and astrophysics. The decays studied were selected primarily because they have a large impact on the prediction of a) the decay heat in reactors, important for the safety of present and future reactors and b) the reactor electron antineutrino spectrum, of interest for particle/nuclear physics and reactor monitoring. For these studies the total absorption technique was chosen, since it is the only method that allows one to obtain beta decay probabilities free from a systematic error called the Pandemonium effect. The me…

safetyNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaPenning trapFOS: Physical sciencesnucleus: structure functionnuclear model[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energylaw.inventionNuclear physicslawnuclear physics0103 physical sciencesNuclear fusionNeutronDecay heatNuclear Experiment (nucl-ex)n: capture010306 general physicsNuclear ExperimentNuclear ExperimentPhysicsantineutrino: spectrum010308 nuclear & particles physicsPandemonium effectsemileptonic decayNuclear reactorNeutron capturemonitoring13. Climate actionnuclear reactorDelayed neutronElectron neutrinoabsorptionThe European Physical Journal A
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