Search results for "neutron [Stars]"

showing 10 items of 932 documents

Molecular association of cryptand 221D in NaCl-water solutions. A small-angle neutron scattering study

1993

Molecules of 5-Decyl-4,7,13,16,21-pentaoxa-1,10-diaza-bicyclo-[8.8.5.]tricosan (221D) and its sodium complex, with both a hydrophobic and a hydrophilic portion, are expected to form aggregates in water solutions. This was confirmed by surface tension measurements. The aggregation behaviour was studied by small-angle neutron scattering at two different [NaCl]/[221D] molar ratios, such as to obtain, in one case, aggregates entirely made up of ionic monomers, and in the other, mixed micelles constituted by both ionic and non-ionic units. The variation of the aggregation number and number of aggregates indicated that, in the former case, smaller micelles were formed, as a consequence of repulsi…

010302 applied physicsAggregation numberAqueous solutionChemistryCryptandGeneral Physics and AstronomyIonic bonding02 engineering and technologyNeutron scattering021001 nanoscience & nanotechnology01 natural sciencesMicelleSmall-angle neutron scatteringSurface tensionCrystallography[PHYS.HIST]Physics [physics]/Physics archives0103 physical sciences0210 nano-technologyLe Journal de Physique IV
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Neutron scattering and imaging: a tool for archaeological studies

2015

International audience; Neutron scattering and neutron imaging are powerful techniques for studying the structure of objects without damage, which is an essential prerequisite for investigations in Cultural Heritage domain, particularly in Archaeology. The deep penetration of neutrons in most materials allows for the study of relatively large objects. The contrast between similar materials, like metals in alloys, or that due to the presence of hydrogen atoms gives information about the internal structure of objects that have been modified or repaired in the past. Imaging and tomography give a 3-dimensional view of the whole object, permitting discrimination between different parts of the ob…

010302 applied physicsElemental compositionMaterials sciencebusiness.industryNeutron imagingneutron scatteringDeep penetrationQuantitative EvaluationsStructure02 engineering and technologyNeutron scattering021001 nanoscience & nanotechnology01 natural sciencesArchaeology[SPI]Engineering Sciences [physics]OpticsArchaeologyGeochemistry and PetrologyNeutron imaging0103 physical sciencesNeutronPorous materialsTomography0210 nano-technologybusiness
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Effects of Thermal Neutron Irradiation on a Self-Refresh DRAM

2020

International audience; In this study, static and dynamic test methods were used to define the response of a self-refresh DRAM under thermal neutron irradiation. The neutron-induced failures were investigated and characterized by event cross-sections, soft-error rate and bitmaps evaluations, leading to an identification of permanent and temporarily stuck cells, block errors, and single-bit upsets.

010302 applied physicsMaterials science010308 nuclear & particles physicsNuclear engineering01 natural sciencesNeutron temperature[SPI.TRON]Engineering Sciences [physics]/Electronics0103 physical sciences[INFO.INFO-ES]Computer Science [cs]/Embedded SystemsNeutronIrradiation[SPI.NANO]Engineering Sciences [physics]/Micro and nanotechnologies/MicroelectronicsDramBlock (data storage)Dynamic testing2020 15th Design & Technology of Integrated Systems in Nanoscale Era (DTIS)
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EPR and optical spectroscopy of neutron-irradiated Gd3Ga5O12 single crystals

2020

Abstract In this paper, we have performed comparative analysis of EPR, optical absorption (OA) and luminescence spectra for a series of Gd3Ga5O12 (GGG) single crystals irradiated with fast neutrons with fluencies varied from 1016 to 1020n/cm2. In a crystal irradiated with the maximum neutron fluence, the EPR spectra demonstrated the formation of several paramagnetic defects. In particular, EPR spectrum shows a strong resonance at (effective) g ≈ 1.4 with practically isotropic behavior in the crystal rotation around the [1 1 1] direction (magnetic field being perpendicular to [1 1 1]) and several weaker lines in the g ≈ 1.1–2.6 region, which show more pronounced angular dependences. While th…

010302 applied physicsNuclear and High Energy PhysicsMaterials sciencePhotoluminescenceResonance02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesMolecular physicsNeutron temperaturelaw.inventionCrystalParamagnetismlaw0103 physical sciences0210 nano-technologySpectroscopyLuminescenceElectron paramagnetic resonanceInstrumentationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Determination of impurity distributions in ingots of solar grade silicon by neutron activation analysis

2017

AbstractIn a series of crystallization experiments, the directional solidification of silicon was investigated as a low cost path for the production of silicon wafers for solar cells. Instrumental neutron activation analysis was employed to measure the influence of different crystallization parameters on the distribution of 3d-metal impurities of the produced ingots. A theoretical model describing the involved diffusion and segregation processes during the solidification and cooling of the ingots could be verified by the experimental results. By successive etching of the samples after the irradiation, it could be shown that a layer of at least 60 μm of the samples has to be removed to get r…

010302 applied physicsSiliconMetallurgychemistry.chemical_elementdirectional solidification02 engineering and technologysolar silicon021001 nanoscience & nanotechnology01 natural sciencesMaterialien - Solarzellen und TechnologieKristallisation und Waferingtransition metalsSilicium-PhotovoltaikchemistryImpurityPhotovoltaik0103 physical sciencesPhysical and Theoretical ChemistryNeutron activation analysis0210 nano-technologyfeedstockneutron activation analysis
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Inelastic neutron scattering study of proton dynamics in Ca(OH)2 at 20 K

1995

Abstract Inelastic neutron scattering (INS) spectra of Ca(OH) 2 at 20 K are presented from 30 to 4000 cm −1 for a powder sample, from 30 to 12000 cm −1 for an oriented single-crystal. INS band splitting due to the lattice density-of-states is observed. Polarization effects reveal the orientation of atomic displacements for each mode and a new band assignment scheme is proposed. For the single-crystal, the v OH mode and overtones are observed. This oscillator shows only moderate anharmonicity. Spectrum simulation reveals that INS spectral intensities are not consistent with simple normal coordinates and harmonic force-fields for Ca(OH) 2 entities. A new dynamical model is proposed, including…

010304 chemical physicsInfraredChemistryAnharmonicityGeneral Physics and Astronomy02 engineering and technology021001 nanoscience & nanotechnologyPolarization (waves)01 natural sciencesMolecular physicsSpectral lineInelastic neutron scatteringsymbols.namesakeCrystallographyLattice (order)0103 physical sciencessymbolsNormal coordinates[CHIM]Chemical SciencesPhysical and Theoretical Chemistry0210 nano-technologyRaman spectroscopyComputingMilieux_MISCELLANEOUS
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The research reactor TRIGA Mainz – a strong and versatile neutron source for science and education

2019

Abstract The TRIGA Mark II-reactor at the Johannes Gutenberg University Mainz (JGU) is one of three research reactors in Germany. The TRIGA Mainz became first critical on August 3rd, 1965. It can be operated in the steady state mode with a maximum power of 100 kWth and in the pulse mode with a peak power of 250 MWth and a pulse length of 30 ms. The TRIGA Mainz is equipped with a central thimble, a rotary specimen rack, three pneumatic transfer systems, four beam tubes, and a graphite thermal column. The TRIGA Mainz is intensively used both for basic and applied research in nuclear chemistry and nuclear physics. Two sources for ultra-cold neutrons (UCN) are operational at two beam ports. At …

010308 nuclear & particles physicsChemistryNuclear engineering0103 physical sciencesNeutron sourceResearch reactorPhysical and Theoretical Chemistry010306 general physics01 natural sciencesTRIGARadiochimica Acta
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Neutron imaging and tomography: Applications in food science

2018

International audience; Neutron imaging and tomography allow observing the structure of large objects (from few to hundred centimeters) at a resolution around 100 μm. This non-destructive method is based on the detection of the transmission of a neutron beam through an object in 2D (imaging) or 3D after rotating the sample (tomography). The components of the object attenuate the neutron beam differently, depending on their composition, and produce accurate pictures of objects which give information about their structure. Neutron imaging has been used for quality control purposes in industries (aircraft, motor engineering...), but also find application from materials sciences (fuel cells, li…

010308 nuclear & particles physicsNeutron imagingPhysicsQC1-99902 engineering and technologyNeutron radiation021001 nanoscience & nanotechnologyObject (computer science)01 natural sciencesSample (graphics)0103 physical sciencesFuel cellsTomographyFood science0210 nano-technology[SDV.AEN]Life Sciences [q-bio]/Food and NutritionEPJ Web of Conferences
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Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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IGR J17329-2731: The birth of a symbiotic X-ray binary

2018

We report on the results of the multiwavelength campaign carried out after the discovery of the INTEGRAL transient IGR J17329-2731. The optical data collected with the SOAR telescope allowed us to identify the donor star in this system as a late M giant at a distance of 2.7$^{+3.4}_{-1.2}$ kpc. The data collected quasi-simultaneously with XMM-Newton and NuSTAR showed the presence of a modulation with a period of 6680$\pm$3 s in the X-ray light curves of the source. This unveils that the compact object hosted in this system is a slowly rotating neutron star. The broadband X-ray spectrum showed the presence of a strong absorption ($\gg$10$^{23}$ cm$^{-2}$) and prominent emission lines at 6.4 …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesFluxAstrophysicsCompact star01 natural sciencesSpectral linelaw.inventionTelescopeSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsAstronomy and AstrophysicLight curveX-rays: binarieNeutron starX-rays: individuals: IGR J17329-273113. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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