Search results for "Spectral"

showing 10 items of 3116 documents

Multiphoton One-step Ionization of Helium at 1064 nm

1989

Abstract The multiphoton ionization of helium by a strong radiation field having a wavelength of 1064 nm and a field intensity up to 5 × 1014 W cm −2 is considered within a non-perturbative treatment partially accounting for the electron-electron correlations in the initial bound state and approximately for the Coulomb interaction between the residual ion and the ejected electron in the final state. Only single-electron transitions are considered, the main emphasis being on the field polarization effects. The obtained results are compared with the few results available in the literature in the same regime as well as with very recent experimental findings. In particular, the calculated photo…

PhysicsWavelengthchemistryIonizationBound statechemistry.chemical_elementElectronAtomic physicsPolarization (waves)Atomic and Molecular Physics and OpticsSpectral lineHeliumIonJournal of Modern Optics
researchProduct

The use of the integral-bias summing coincidence spectrometer in directional correlation measurements

1968

Abstract The performance of the integral-bias summing coincidence spectrometer (the sum-peak spetrometer) in measurements of directional correlations of gamma rays has been tested. As compared with the conventional method, the sum-peak spectrometer is easier to use and seems to yield results which agree with those obtained with the ordinary method. Because of the complex shapes of response functions of gamma rays above about 3 MeV, the new method is best suited to the study of cascading transitions below this energy, where the two methods appear to complement each other. The analysis of the sum-peak spectra in the present work is based on a simple graphical method which seems to yield satis…

PhysicsWork (thermodynamics)Spectrometer010308 nuclear & particles physicsGamma rayGeneral Medicine01 natural sciencesCoincidenceSpectral lineNuclear physicsYield (chemistry)0103 physical sciences010306 general physicsEnergy (signal processing)Complement (set theory)Nuclear Instruments and Methods
researchProduct

Element-specific magnetic moments and spin-resolved density of states in CoFeMnZ(Z=Al, Ga; Si, Ge)

2011

Using circular dichroism in x-ray-absorption spectroscopy (XAS/XMCD), we determined element-specific magnetic moments and spin-resolved unoccupied densities of states (DOS) for Co, Fe, and Mn in the quaternary Heusler compounds CoFeMn$Z$ ($Z=\text{Al}$, Ga; Si, Ge). These compounds belong to a class of highly spin-polarized materials with cubic LiMgPdSn-type structure. Different structure models for the sublattice occupation leading to similar average magnetization values can be distinguished by comparison of element-specific moments with theory. We find that the compounds form similar structures, where Co, Fe, Mn, and $Z$ occupy the $X$, ${X}^{\ensuremath{'}}$, $Y$, and $Z$ sublattice of t…

PhysicsX-ray absorption spectroscopyMagnetizationCircular dichroismMagnetic momentCondensed matter physicsDensity of statesAtomic physicsCondensed Matter PhysicsSpin (physics)SpectroscopySpectral lineElectronic Optical and Magnetic MaterialsPhysical Review B
researchProduct

The Sax Mission for X-Ray Astronomy

1990

The satellite for X-ray astronomy SAX, to be launched at the end of 1993, is devoted to systematic, integrated and comprehensive, studies of galactic and extra-galactic sources in the energy band 0.1–200 keV, and is under joint development by the Italian Space Agency (ASI) and the Netherlands Agency for Aerospace programs (NIVR), with the participation of SRU/SRON and SSD/ESTEC. The basic scientific objectives can be summarized as follows: — Broad band spectroscopy (E/△ E=12) from 0.1–10 keV with imaging resolution of 1 arcmin. — Continuum and line spectroscopy (E/△ E=5-20) in the energy range 3–200 keV. — Variability studies of bright source energy spectra on timescales from milliseconds t…

PhysicsX-ray astronomyEinstein TelescopeSkyAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectX-ray detectorBroad bandAstronomyAstrophysicsSpectroscopySpectral linemedia_common
researchProduct

X-ray and gamma-ray astronomy with NTD germanium-based microcalorimeters

2002

We report on the performance of our NTD-Ge microcalorimeters. To date, the spectral resolution for x-ray and gamma-ray lines from radioactive sources and laboratory plasmas is 4.8 eV in the entire 1 - 6 keV band and 52 eV at 60 keV. Technical details responsible for this performance are presented as well as an innovative electro-thermal approach for enhancing count-rate capability.

PhysicsX-ray astronomyX-raychemistry.chemical_elementGermaniumPlasmaGamma-ray astronomyAstrophysicsmicrocalorimeterlaw.inventionX-rayAstrophysicGermanium radiation detectorsSettore FIS/05 - Astronomia E AstrofisicachemistrylawNTD Germaniumgamma-raySpectral resolutionLight-emitting diode
researchProduct

A Preliminary Analysis of a New Chandra Observation (ObsID 6148) of Cir X-1

2008

We present the preliminary spectral analysis of a 25 ks long Chandra observation of the peculiar source Cir X–1 near the periastron passage. We estimate more precise coordinates of the source compatible with the optical and radio counterpart coordinates. We detect emission lines associated to Mg XII, Si XIII, Si XIV, S XV, S XVI Ar XVII, Ar XVIII, Ca XIX, Ca XX, Fe XXV, Fe XXVI showing a redshift of 470 km s−1. The more intense emission features at 6.6 keV show a double‐peaked shape that can be modelled with two or three Gaussian lines.

PhysicsX-ray binaries Accretion and accretion disks Neutron stars Distances redshifts radial velocities; spatial distribution of galaxies Black holesX-ray binaries Accretion and accretion disks Neutron stars Distances redshifts radial velocitieGaussianX-ray binaryAstronomyAstrophysicsRedshiftPreliminary analysisRed shiftNeutron starsymbols.namesakeSettore FIS/05 - Astronomia E AstrofisicasymbolsSpectral analysisEmission spectrumspatial distribution of galaxies Black holes
researchProduct

The BeppoSAX 0.1–18 keV spectrum of the bright atoll source GX 9+1: an indication of the source distance

2005

We report the results of a long, 350 ks, BeppoSAX observation of the bright atoll source GX 9+1 in the 0.12-18 keV energy range. During this observation GX 9+1 showed a large count rate variability in its lightcurve. From its color-color diagram we selected six zones and extracted the source energy spectrum from each zone. We find that the model, composed of a blackbody plus a Comptonized component absorbed by an equivalent hydrogen column of ~1.4 ¿ 1022 cm-2, fits the spectra in the energy range 1-18 keV well; however, below 1 keV a soft excess is present. We find that the spectrum of GX 9+1, in the 0.12-18 keV energy range, is well fitted by the model above, if we use an equivalent hydrog…

PhysicsX-ray binaryAstronomyAstronomy and AstrophysicsAstrophysicsLight curveSpectral lineLuminosityInterstellar mediumNeutron starStarssymbols.namesakeSpace and Planetary ScienceEddington luminositysymbolsAstronomy & Astrophysics
researchProduct

High-Energy pulse profile of the Transient X-ray Pulsar SAX J2103.5+4545

2005

In two recent INTEGRAL papers, Lutovinov et al. (2003) and Blay et al. (2004) report a timing and spectral analysis of the transient Be/X-ray pulsar SAX J2103.5+4545 at high energies (5--200 keV). In this work we present for the first time a study of the pulse profile at energies above 20 keV using INTEGRAL data. The spin-pulse profile shows a prominent (with a duty cycle of 14%) and broad (with a FWHM of ~ 51 s) peak and a secondary peak which becomes more evident above 20 keV. The pulsed fraction increases with energy from ~ 45% at 5--40 keV to ~ 80% at 40--80 keV. The morphology of the pulse profile also changes as a function of energy, consistent with variations in the spectral componen…

PhysicsX-rays : binariesScatteringAstrophysics::High Energy Astrophysical Phenomenapulsars : individual : SAX J2103.5+4545Astrophysics (astro-ph)Phase (waves)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsRadiationAstrophysicsSpectral linePulse (physics)Full width at half maximumPulsarbinaries : closeSpace and Planetary Scienceclose; pulsars : individual : SAX J2103.5+4545; X-rays : binaries [binaries]X-ray pulsar
researchProduct

An X-shooter survey of star forming regions: Low-mass stars and sub-stellar objects

2011

We present preliminary results of our X-shooter survey in star forming regions. In this contribution we focus on sub-samples of young stellar and sub-stellar objects (YSOs) in the Lupus star forming region and in the TW Hya association. We show that the X-shooter spectra are suitable for conducting several parallel studies such as YSO + disk fundamental parameters, accretion and outflow activity in the very low-mass (VLM) and sub-stellar regimes, as well as magnetic activity in young VLM YSOs, and Li abundance determinations. The capabilities of X-shooter in terms of wide spectral coverage, resolution and limiting magnitudes, allow us to assess simultaneously the accretion/outflow, magnetic…

PhysicsYoung stellar objectBrown dwarfAstronomyAstronomy and AstrophysicsAstrophysicsAccretion (astrophysics)Spectral lineT Tauri starStarsaccretion accretion disks ISM: jets and outflows stars: formation stars: low-mass brown dwarfs stars: pre-main sequence T Tauri starsSpace and Planetary ScienceOutflowLow Massjets and outflows stars: formation stars: low-mass brown dwarfs stars: pre-main sequence T Tauri stars [accretion accretion disks ISM]
researchProduct

Bose condensates at high angular momenta

2000

We exploit the analogy with the Quantum Hall (QH) system to study weakly interacting bosons in a harmonic trap. For a $\delta$-function interaction potential the ``yrast'' states with $L\ge N(N-1)$ are degenerate, and we show how this can be understood in terms of Haldane exclusion statistics. We present spectra for 4 and 8 particles obtained by numerical and algebraic methods, and demonstrate how a more general hard-core potential lifts the degeneracies on the yrast line. The exact wavefunctions for N=4 are compared with trial states constructed from composite fermions (CF), and the possibility of using CF-states to study the low L region at high N is discussed.

PhysicsYrastDegenerate energy levelsCondensed Matter (cond-mat)FOS: Physical sciencesCondensed MatterQuantum Hall effectAtomic and Molecular Physics and OpticsSpectral lineQuantum mechanicsComposite fermionAlgebraic numberWave functionBoson
researchProduct