Search results for "neutron"

showing 10 items of 2330 documents

Structural investigation of hybrid nanocomposites

2002

Ultra small (USANS) and small angle neutron scattering (SANS) techniques were employed to study an elastomer styrene–butadiene, where two kinds of silica fillers have been added in different amounts. Small silica-particle fillers are expected to modify morphological and mechanical properties when dispersed in the copolymer matrix. The USANS and SANS techniques can span a wide range of momentum transfer, investigating morphological properties of the filled elastomer over a number of decades in length scale. Surface and mass fractal behavior has been observed over different length scales.

Length scaleMaterials scienceNanocompositeMomentum transferGeneral ChemistryElastomerSmall-angle neutron scatteringMatrix (geology)Condensed Matter::Soft Condensed MatterCondensed Matter::Materials ScienceFractalCopolymerGeneral Materials ScienceComposite materialApplied Physics A: Materials Science & Processing
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Small Angle Neutron Scattering, X-ray Diffraction, Differential Scanning Calorimetry, and Thermogravimetry Studies to Characterize the Properties of …

2009

Nanocomposites based on laponite RD and (ethylene oxide)98(propylene oxide)67(ethylene oxide)98 (F127)triblock copolymer or poly(ethylene) glycol 2000 (PEG2000) were prepared by using the melting method. Small-angle neutron scattering and the X-ray diffraction experiments provided insights into the organization of the laponite RD dispersed in the macromolecular matrix over a wide length scale. SANS data analysis by means of a fractal law evidenced the formation of clusters of laponite RD at long correlation distance. The single laponite RD particles and the lamellar structure of F127 were described in the shorter length scale. Finally, the crystalline structure of the macromolecule was obse…

Length scaleTGAMaterials scienceEthylene oxidenanocompositepoly(ethylene oxide)poly(propylene oxide)poly(ethylene oxide)SANSXRDAnalytical chemistrypoly(ethylene)glycol 2000laponite RDNeutron scatteringSmall-angle neutron scatteringSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsDSCThermogravimetrychemistry.chemical_compoundGeneral EnergyDifferential scanning calorimetrychemistryX-ray crystallographyLamellar structurePhysical and Theoretical Chemistry
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Structural Organization of Poly(vinyl alcohol) Hydrogels Obtained by Freezing and Thawing Techniques:  A SANS Study

2005

The structural organization of matter in poly(vinyl alcohol) (PVA) hydrogels obtained by repeatedly freezing and thawing dilute solutions of PVA in D2O is investigated by use of small-angle neutron scattering measurements (SANS). This study is the first systematic and quantitative investigation in the medium range of length scales on PVA hydrogels obtained by freezing and thawing techniques. The studied gels have a complex hierarchical structure, extending over a wide range of length scales. The structural organization on the micron length scale originates from the presence of two separated phases constituted by polymer-rich and polymer-poor regions. The network structure may be interpreted…

Length scaleVinyl alcoholMaterials sciencenanostructureGeneral Chemical EngineeringNeutron scatteringPOLYVINYL-ALCOHOL) GELSGELATION PROCESSchemistry.chemical_compoundPhase (matter)AQUEOUS-SOLUTIONSPolymer chemistryMaterials ChemistrySMALL-ANGLE NEUTRONStructural organizationGeneral ChemistryLIGHT-SCATTERINGCondensed Matter::Soft Condensed MatterChemical engineeringchemistryMedium rangeSelf-healing hydrogelsSmall-angle neutron scatteringMORPHOLOGYCrystallitehydrogelPHASE-SEPARATIONChemistry of Materials
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Phenol compounds as a New Materials for EPR dosimetry in radiation therapy

2016

Among the various dosimetric techniques used for characterizing the radiation beams used in radiation therapy, the Electron Paramagnetic Resonance (EPR) arouses increasing interest for applications in various therapy procedures. When a compound is irradiated with ionizing radiations free radicals are produced and their concentration is proportional to the absorbed dose. This allows for dosi-metric measurements through EPR technique which is able to quantitatively de-termine the radical concentration. Our research group has started an investigation of the EPR response of some phenols compounds for possible dosimetric applications. In this work we report the EPR investigation of IRGANOX 1076 …

LinacSettore FIS/01 - Fisica SperimentalePhenols ESR EPR Dosimetry Neutron GammaSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Settore CHIM/02 - Chimica Fisica
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HOW TO MAKE LIQUID METAL TRANSPARENT? A NEUTRON RADIOGRAPHY METHOD FOR SCALED-DOWN METALLURGICAL EQUIPMENT

2016

Liquid metalMaterials scienceNeutron imagingMetallurgyProceeding of First Thermal and Fluids Engineering Summer Conference
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Numerical and experimental study of liquid metal stirring by rotating permanent magnets

2018

In this work, we study liquid gallium stirring by rotating permanent magnets. We demonstrate possibility of easily creating different flow patterns by rotating permanent magnets, which can be industrially important for controlling heat and mass transfer processes in the system. Unlike the typical approach of simulating magnet rotation as a transient problem and time-averaging the Lorentz forces, we solve the magnet rotation as a harmonic (frequency domain) problem, which leads to forces equal to time-averaged ones and decreases the simulation time considerably. Numerical results are validated using qualitative flow structure results from the neutron radiography visualization of tracer parti…

Liquid metalMaterials sciencePermanent magnetsNumerical modelsUltrasonic Doppler velocimeters02 engineering and technologyQuantitative dataRotationHeat and mass transfer process020501 mining & metallurgyPhysics::Fluid DynamicsMagnetohydrodynamicssymbols.namesakeFrequency domainsneutron radiographyLiquid metal stirringTransient problemsFrequency domain analysisddc:530Mass transferUDVMagnetic materialsMetal meltingNumerical and experimental studyData visualizationnumerical modellingMechanicsVelocimetry0205 materials engineeringFrequency domainMagnetNumerical resultsHarmonicsymbolsUltrasound Doppler velocimetryDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikTransient (oscillation)Lorentz forceLiquid metalsIOP Conference Series: Materials Science and Engineering
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Triplet 12B-12C-12N : Search for States with Halo

2020

Previously in [1] neutron halo was confirmed for the 2¯, 1.67 MeV and 1¯, 2.62 MeV states in 12B on base of Asymptotic Normalization Coefficients (ANC) method analysis of the obtained experimental data. An unexpected result was received for the unbound 3¯, 3.39 MeV state. Its halo radius was found to be increased and equal to ~5.9 fm. This result can be considered as an evidence of the halo-like structure in this 12B state. It should be noted that last neutron in this state has a non-zero orbital momentum (l = 2). So question arises about possible existence of states with halo in other members of the isobaric triplet 12B–12C–12N. We can expect the formation of a proton halo in the 2¯, 1.19 …

MDM modelNuclear Theoryasymptotic normalization coefficients neutron and proton haloradii of excited statesNuclear Experiment
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Multimessenger search for sources of gravitational waves and high-energy neutrinos: Initial results for LIGO-Virgo and IceCube

2014

Made available in DSpace on 2022-04-29T07:21:49Z (GMT). No. of bitstreams: 0 Previous issue date: 2014-11-17 We report the results of a multimessenger search for coincident signals from the LIGO and Virgo gravitational-wave observatories and the partially completed IceCube high-energy neutrino detector, including periods of joint operation between 2007-2010. These include parts of the 2005-2007 run and the 2009-2010 run for LIGO-Virgo, and IceCube's observation periods with 22, 59 and 79 strings. We find no significant coincident events, and use the search results to derive upper limits on the rate of joint sources for a range of source emission parameters. For the optimistic assumption of …

MECHANISMPhysics and Astronomy (miscellaneous)AstrophysicsFOLLOW-UP OBSERVATIONSASTROPHYSICAL SOURCESIceCubeneutrinoDetection of gravitational waveGravitational waves neutrinoObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QCLIGO Scientific CollaborationQBPhysicsGAMMA-RAY BURSTS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsASTRONOMYNuclear and High Energy Physics; Physics and Astronomy (miscellaneous)NEUTRINOSNeutrino detectorComputingMethodologies_DOCUMENTANDTEXTPROCESSINGNeutrinoSENSITIVITYGIANT FLARENuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]95.85.RyMUON NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATIONGravitational wavesGeneral Relativity and Quantum CosmologyINSTABILITIESSettore FIS/05 - Astronomia e AstrofisicaCORE-COLLAPSE SUPERNOVAE[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530SDG 7 - Affordable and Clean EnergyCORE-COLLAPSEDETECTOR/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyGravitational wave95.85.SzMAGNETIZED NEUTRON-STARS[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AstronomyTRANSIENTS95.85.Sz; 95.85.RyRELATIVISTIC STARSLIGOPhysics and Astronomy[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Gamma-ray burstEMISSIONEnergy (signal processing)
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The force-free twisted magnetosphere of a neutron star

2016

We present a detailed analysis of the properties of twisted, force-free magnetospheres of non-rotating neutron stars, which are of interest in the modelling of magnetar properties and evolution. In our models the magnetic field smoothly matches to a current-free (vacuum) solution at some large external radius, and they are specifically built to avoid pathological surface currents at any of the interfaces. By exploring a large range of parameters, we find a few remarkable general trends. We find that the total dipolar moment can be increased by up to $40\%$ with respect to a vacuum model with the same surface magnetic field, due to the contribution of magnetospheric currents to the global ma…

MHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesMagnetosphere7. Clean energy01 natural sciences010305 fluids & plasmasNuclear physicsmagnetars [Stars]0103 physical sciencesmedia_common.cataloged_instanceCost actionEuropean union010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)media_commonAstronomía y AstrofísicaHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and Astrophysicsneutron [Stars]Magnetic fieldNeutron starAstrophysics - Solar and Stellar AstrophysicsWork (electrical)Space and Planetary ScienceMagnetic fieldsMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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How to form a millisecond magnetar? Magnetic field amplification in protoneutron stars

2017

Extremely strong magnetic fields of the order of $10^{15}\,{\rm G}$ are required to explain the properties of magnetars, the most magnetic neutron stars. Such a strong magnetic field is expected to play an important role for the dynamics of core-collapse supernovae, and in the presence of rapid rotation may power superluminous supernovae and hypernovae associated to long gamma-ray bursts. The origin of these strong magnetic fields remains, however, obscure and most likely requires an amplification over many orders of magnitude in the protoneutron star. One of the most promising agents is the magnetorotational instability (MRI), which can in principle amplify exponentially fast a weak initia…

MHD[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsmagnetic fieldsMagnetar01 natural sciencesstars: neutronsupernovae: generalstars: rotation0103 physical sciencesstars: magnetic fieldsAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMillisecond010308 nuclear & particles physicsAstronomy and AstrophysicsMagnetic fieldStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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