Search results for "design [electronics]"

showing 10 items of 505 documents

Properties of the isolated neutron star RX J185635-3754

2004

Abstract Despite improved observational capabilities, the surface properties of neutron stars remain uncertain. In principle, multiwavelength spectra can reveal their compositions and angular diameters and constrain the interior equation of state. The Chandra LETG spectrum of the brightest isolated neutron star is a featureless continuum. The X-ray blackbody fit underpredicts the observed optical fluxes, but the spectral energy distribution can be fit with a two blackbody model. No pulsations are seen. We discuss model atmosphere fits. We conclude there is no need to invoke exotic physics: RX J185635-3754 is likely a 0.5 × 10 6 years old pulsar.

PhysicsAtmospheric ScienceEquation of stateAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)Aerospace EngineeringAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSpectral lineAtmosphereNeutron starGeophysicsPulsarSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsGeneral Earth and Planetary SciencesSpectral energy distributionBlack-body radiationAdvances in Space Research
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Long Lived Acoustic Vibrational Modes of an Embedded Nanoparticle

2004

Classical continuum elastic calculations show that the acoustic vibrational modes of an embedded nanoparticle can be lightly damped even when the longitudinal plane wave acoustic impedances $Z_o=\rho v_L$ of the nanoparticle and the matrix are the same. It is not necessary for the matrix to be less dense or softer than the nanoparticle in order to have long lived vibrational modes. Continuum boundary conditions do not always accurately reflect the microscropic nature of the interface between nanoparticle and matrix, and a multi-layer model of the interface reveals the possibility of additional reduction of mode damping.

PhysicsCondensed Matter - Materials ScienceContinuum (design consultancy)Materials Science (cond-mat.mtrl-sci)FOS: Physical sciencesGeneral Physics and AstronomyNanoparticle[ PHYS.COND.CM-GEN ] Physics [physics]/Condensed Matter [cond-mat]/Other [cond-mat.other]Molecular physicsMatrix (mathematics)Classical mechanicsMolecular vibrationBoundary value problemReduction (mathematics)Acoustic impedanceElectrical impedancePhysical Review Letters
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Magnetic-field-enhanced outgoing excitonic resonance in multi-phonon Raman scattering from polar semiconductors

1996

A combined scattering mechanism involving the states of free electron-hole pairs (exciton continuum) and discrete excitons as intermediate states in the multi-phonon Raman scattering leads to (1) a strong increase of the scattering efficiency in the presence of a high magnetic field and to (2) an outgoing excitonic resonance: the two features are not compatible when only free pairs (leading to a strong increase of the scattering efficiency under the applied magnetic field) or discrete excitons (resulting in the outgoing resonance at the excitonic gap) are taken into account.

PhysicsCondensed Matter::OtherPhononScatteringExcitonCondensed Matter (cond-mat)Continuum (design consultancy)FOS: Physical sciencesCondensed MatterCondensed Matter::Mesoscopic Systems and Quantum Hall EffectCondensed Matter PhysicsMolecular physicsResonance (particle physics)Magnetic fieldCondensed Matter::Materials Sciencesymbols.namesakesymbolsPolarGeneral Materials ScienceRaman scatteringJournal of Physics: Condensed Matter
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Phototransition of Na(3p3/2) into high Rydberg states and the ionization continuum

2005

A model potential method is used to investigate photoabsorption from the Na(3p3/2) state. Absorption cross sections into higher Rydberg states and photoionization cross sections are presented as an analytical function of photo electron energy. Einstein coefficients for spontaneous emissions 3p3/2 ← ns1/2, nd5/2, nd3/2 are tabulated for n up to 50. The Einstein coefficients and low-energy ionization cross sections are believed to be accurate to better than 2–3%, above 1 eV the error may increase to 4–6%.

PhysicsElectron energyContinuum (design consultancy)PhotoionizationCondensed Matter PhysicsAtomic and Molecular Physics and Opticssymbols.namesakeEinstein coefficientsIonizationPhysics::Atomic and Molecular ClustersRydberg formulasymbolsSpontaneous emissionAtomic physicsAbsorption (electromagnetic radiation)Journal of Physics B: Atomic, Molecular and Optical Physics
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New VR magnification ratios of QSO 0957+561

2004

We present VR magnification ratios of QSO 0957+561, which are inferred from the GLITP light curves of Q0957+561A and new frames taken with the 2.56m Nordic Optical Telescope about 14 months after the GLITP monitoring. From two photometric approaches and a reasonable range for the time delay in the system (415-430 days), we do not obtain achromatic optical continuum ratios, but ratios depending on the wavelength. These new measurements are consistent with differential extinction in the lens galaxy, the Lyman limit system, the damped Ly-alpha system, or the host galaxy of the QSO. The possible values for the differential extinction and the ratio of total to selective extinction in the V band …

PhysicsExtinction (astronomy)Continuum (design consultancy)Astrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLight curveGravitational microlensingAstrophysicsGalaxyLyman limitNordic Optical TelescopeWavelengthSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy Astrophysics
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Coincidence Electron Scattering (e, e′c) in the Giant Resonance Region of 28Si

1986

In the nuclear continuum region, the inherent power of inelastic electron scattering to map out the Fourier transforms of the transition charge and current densities is completely exploited only if the inelastically scattered electron is detected in coincidence with a nuclear decay product c. The coincidence requirement effectively eliminates the strong elastic radiative tail which hitherto plagued the analysis of single arm (e,e′) experiments.

PhysicsGiant resonanceContinuum (design consultancy)Radiative transferElectronMott scatteringAtomic physicsElectron scatteringCoincidenceRadioactive decay
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Radio emission of SN1993J: the complete picture. I. Re-analysis of all the available VLBI data

2010

We have performed a complete re-calibration and re-analysis of all the available VLBI observations of supernova SN1993J, following an homogeneous and well-defined methodology. Observations of SN1993J at 69 epochs, spanning 13 years, were performed by two teams, which used different strategies and analysis tools. The results obtained by each group are similar, but their conclusions on the supernova expansion and the shape and evolution of the emitting region differ significantly. From our analysis of the combined set of observations, we have obtained an expansion curve with unprecedented time resolution and coverage. We find that the data from both teams are compatible when analyzed with the…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Spectral indexCosmology and Nongalactic Astrophysics (astro-ph.CO)OpacityAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxySupernovaWavelengthSpace and Planetary ScienceVery-long-baseline interferometryAstrophysics - High Energy Astrophysical PhenomenaEjectaAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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A re-analysis of the NuSTAR and XMM-Newton broad-band spectrum of Serpens X-1

2017

Context. High-resolution X-ray spectra of neutron star low-mass X-ray binaries (LMXBs) in the energy range 6.4-6.97 keV are often characterized by the presence of K alpha transition features of iron at different ionization stages. Since these lines are thought to originate by reflection of the primary Comptonization spectrum over the accretion disk, the study of these features allows us to investigate the structure of the accretion flow close to the central source. Thus, the study of these features gives us important physical information on the system parameters and geometry. Ser X-1 is a well studied LMXB that clearly shows a broad iron line. Several attempts to fit this feature as a smear…

PhysicsLine-of-sight010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)Astronomy and AstrophysicsContext (language use)RadiusAstrophysicsX-rays: general01 natural sciencesX-rays: binarieSpectral linestars: neutronQuality (physics)Reflection (mathematics)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Science0103 physical sciencesstars: individual: Serpens X-1formation; line: identification; stars: individual: Serpens X-1; stars: neutron; X-rays: binaries; X-rays: general [line]line: formation010303 astronomy & astrophysicsline: identificationLine (formation)
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Breakup channels forC12triple-αcontinuum states

2009

The triple-alpha-particle breakup of states in the triple-alpha continuum of C-12 has been investigated by way of coincident detection of all three alpha particles of the breakup. The states have been fed in the beta decay of N-12 and B-12, and the alpha particles measured using a setup that covers all of the triple-alpha phase space. Contributions from the breakup through the Be-8(0(+)) ground state as well as other channels-interpreted as breakup through excited energies in Be-8-have been identified. Spins and parities of C-12 triple-alpha continuum states are deduced from the measured phase-space distributions for breakup through Be-8 above the ground state by comparison to a fully symme…

PhysicsNuclear and High Energy PhysicsAngular momentumExcited stateNuclear TheoryContinuum (design consultancy)Carbon-12Alpha particleAtomic physicsNuclear ExperimentSpin (physics)Ground stateBreakupPhysical Review C
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Measurement of the inclusive branching fraction for ψ(3686)→KS0+anything

2021

Abstract Using 5.9 pb−1 of e + e − annihilation data collected at center-of-mass energies from 3.640 to 3.701 GeV with the BESIII detector at the BEPCII Collider, we measure the observed cross sections of e + e − → K S 0 X (where X = anything ). From a fit to these observed cross sections with the sum of continuum and ψ ( 3686 ) and J / ψ Breit-Wigner functions and considering initial state radiation and the BEPCII beam energy spread, we obtain for the first time the product of ψ ( 3686 ) leptonic width and inclusive decay branching fraction Γ ψ ( 3686 ) e e B ( ψ ( 3686 ) → K S 0 X ) = ( 373.8 ± 6.7 ± 20.0 ) eV, and assuming Γ ψ ( 3686 ) e e is ( 2.33 ± 0.04 ) keV from PDG value, we measur…

PhysicsNuclear and High Energy PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionContinuum (design consultancy)01 natural sciencesMeasure (mathematics)law.inventionNuclear physicslaw0103 physical sciences010306 general physicsColliderBeam energyPhysics Letters B
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