Search results for " NEUTRON"

showing 10 items of 618 documents

Comment on “Comparison of Polarization Observables in Electron Scattering from the Proton and Deuteron”

1998

PhysicsNuclear physicsProtonDeuteriumPolarization observablesGeneral Physics and AstronomyMott scatteringInelastic scatteringSmall-angle neutron scatteringElectron scatteringPhysical Review Letters
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Model-independent DWBA-analysis of inelastic electron scattering data

2008

PhysicsNuclear physicsResonant inelastic X-ray scatteringElastic scatteringQuasielastic scatteringX-ray Raman scatteringScatteringMott scatteringInelastic scatteringInelastic neutron scattering
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Independent Fission Yield Measurements

1986

Various methods to measure independent yields are reviewed and discussed. A survey on actual measurements carried out after 1978 is given.

PhysicsNuclear reaction010308 nuclear & particles physics0211 other engineering and technologiesMeasure (physics)02 engineering and technologyFission product yield01 natural sciencesNuclear physicsNuclear Energy and Engineering0103 physical sciencesNeutron021108 energyFission neutronDelayed neutronNuclear Science and Engineering
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Searching for the 5H resonance in the t+n+n system

2003

19 pages, 7 figures, 2 tables, 2 appendices.-- PACS nrs.: 27.10.+h; 25.60.Gc.-- Printed version published Jul 28, 2003.

PhysicsNuclear reactionNuclear and High Energy PhysicsComparisons with previous resultsMeasured triton and neutron relative energy spectra energy and angular correlationsHyperspherical harmonic expansion analysisResonance[PACS] Properties of specific nuclei listed by mass ranges: A ≤ 5Nuclear Reactions C(6Hent) (6He2nt) E=240 MeV/nucleonNuclear physicsNuclear magnetic resonanceA ≤ 5 [[PACS] Properties of specific nuclei listed by mass ranges]45H deduced resonance features[PACS] Breakup and momentum distributionsNuclear Physics A
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Low-spin mixed particle–hole structures in 185W

2005

Abstract The level structure of 185W has been studied using the prompt and delayed gamma–gamma coincidences from thermal neutron capture in 184W accompanied with the one-nucleon transfer reactions ( d , p ) and ( d , t ) with polarized beams. From these data and those of previous studies a total of 183 levels has been established for energies below 3 MeV. Many of these states have been grouped into rotational bands built on 28 intrinsic states of quasiparticle and quasiparticle-plus-phonon character. Although the DWBA analysis permitted definite spin–parity assignments for most of states a large number of particle transitions have ‘anomalous’ angular and asymmetry shapes with respect to the…

PhysicsNuclear reactionNuclear and High Energy PhysicsPhononmedia_common.quotation_subjectThermal neutron captureFermi surfaceAsymmetryFragmentation (mass spectrometry)QuasiparticleLevel structureAtomic physicsNuclear Experimentmedia_commonNuclear Physics A
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Small Angle Neutron Scattering from Systems of Interacting Particles. Modelling High Density Micellar Fluids

1992

The need for analytical solutions of the scattering equation for complex situations (polydisperse samples, scattering from non centrosymmetrical particles, etc.) has somehow escaped the attention of the workers in the Small Angle Scattering field, although it is clear that, at the level of sophistication today available for the experiments, a more rigorous approach is necessary. For quite a few years our group has been actively engaged in SANS research and has occasionally devoted its attention to develop alternative ways of data analysis based on more rigorous solutions of the scattering equation.

PhysicsOpticsField (physics)Scatteringbusiness.industryStructure functionHigh densitySmall-angle scatteringbusinessAtomic packing factorRadial distribution functionSmall-angle neutron scatteringComputational physics
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Timing of the 2008 outburst of SAX J1808.4–3658 with XMM-Newton: a stable orbital-period derivative over ten years

2009

We report on a timing analysis performed on a 62-ks long XMM-Newton observation of the accreting millisecond pulsar SAX J1808.4-3658 during the latest X-ray outburst that started on September 21, 2008. By connecting the time of arrivals of the pulses observed during the XMM observation, we derived the best-fit orbital solution and a best-fit value of the spin period for the 2008 outburst. Comparing this new set of orbital parameters and, in particular, the value of the time of ascending-node passage with the orbital parameters derived for the previous four X-ray outbursts of SAX J1808.4-3658 observed by the PCA on board RXTE, we find an updated value of the orbital period derivative, which …

PhysicsOrbital elementsAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesSecular evolutionAstronomy and AstrophysicsAstrophysicsDerivativeOrbital periodstars: neutron stars: magnetic fields X-rays: binaries X-rays: individuals: SAX J1808.4-3658Astrophysics - Astrophysics of GalaxiesLuminosityNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstronomy & Astrophysics
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Timing of the accreting millisecond pulsar SAX J1748.9-2021 during its 2015 outburst

2016

We report on the timing analysis of the 2015 outburst of the intermittent accreting millisecond X-ray pulsar SAX J1748.9-2021 observed on March 4 by the X-ray satellite XMM-Newton. By phase-connecting the time of arrivals of the observed pulses, we derived the best-fit orbital solution for the 2015 outburst. We investigated the energy pulse profile dependence finding that the pulse fractional amplitude increases with energy while no significant time lags are detected. Moreover, we investigated the previous outbursts from this source, finding previously undetected pulsations in some intervals during the 2010 outburst of the source. Comparing the updated set of orbital parameters, in particul…

PhysicsOrbital elementsHigh Energy Astrophysical Phenomena (astro-ph.HE)Millisecondneutron; X-rays: binaries; Space and Planetary Science; Astronomy and Astrophysics [Accretion accretion disc; Stars]010308 nuclear & particles physicsGravitational waveAstrophysics::High Energy Astrophysical PhenomenaAstronomyLagrangian pointFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsOrbital periodX-rays: binarie01 natural sciencesStars: neutronAmplitudePulsarSpace and Planetary ScienceMillisecond pulsar0103 physical sciencesAccretion accretion discAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysics
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Singlet ground state magnetism: II. magnetic excitons in paramagnetic TbP

1979

The magneticΓ 1 –Γ 4 exciton of the singlet ground state system TbP has been studied by inelastic neutron scattering above the antiferromagnetic ordering temperature. Considerable dispersion and a pronounced splitting was found in the [100] and [110] directions. Both the band width and the splitting increased rapidly as the transition temperature was approached in accordance with the predictions of the RPA-theory. The dispersion is analysed in terms of a phenomenological model using interactions up to the fourth nearest neighbour.

PhysicsParamagnetismCondensed matter physicsMagnetismTransition temperatureExcitonPhenomenological modelAntiferromagnetismCondensed Matter PhysicsDispersion (chemistry)Inelastic neutron scatteringElectronic Optical and Magnetic MaterialsZeitschrift f�r Physik B Condensed Matter and Quanta
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Predictions of covariant chiral perturbation theory for nucleon polarisabilities and polarised Compton scattering

2015

We update the predictions of the SU(2) baryon chiral perturbation theory for the dipole polarisabilities of the proton, $\{\alpha_{E1},\,\beta_{M1}\}_p=\{11.2(0.7),\,3.9(0.7)\}\times10^{-4}$fm$^3$, and obtain the corresponding predictions for the quadrupole, dispersive, and spin polarisabilities: $\{\alpha_{E2},\,\beta_{M2}\}_p=\{17.3(3.9),\,-15.5(3.5)\}\times10^{-4}$fm$^5$, $\{\alpha_{E1\nu},\,\beta_{M1\nu}\}_p=\{-1.3(1.0),\,7.1(2.5)\}\times10^{-4}$fm$^5$, and $\{\gamma_{E1E1},\,\gamma_{M1M1},\,\gamma_{E1M2},\,\gamma_{M1E2}\}_p=\{-3.3(0.8),\,2.9(1.5),\,0.2(0.2),\,1.1(0.3)\}\times10^{-4}$fm$^4$. The results for the scalar polarisabilities are in significant disagreement with semi-empirical …

PhysicsParticle physicsChiral perturbation theoryNuclear TheoryPhysics and Astronomy (miscellaneous)ProtonFOS: Physical sciencesCompton scattering Protons and neutron polarisabilitiesNuclear Theory (nucl-th)BaryonHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)PionProduction (computer science)Sensitivity (control systems)Sum rule in quantum mechanicsNucleonEngineering (miscellaneous)The European Physical Journal C
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