572 research outputs found

    Single-photon single ionization of W+^{+} ions: experiment and theory

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    Experimental and theoretical results are reported for photoionization of Ta-like (W+^{+}) tungsten ions. Absolute cross sections were measured in the energy range 16 to 245 eV employing the photon-ion merged-beam setup at the Advanced Light Source in Berkeley. Detailed photon-energy scans at 100 meV bandwidth were performed in the 16 to 108 eV range. In addition, the cross section was scanned at 50 meV resolution in regions where fine resonance structures could be observed. Theoretical results were obtained from a Dirac-Coulomb R-matrix approach. Photoionization cross section calculations were performed for singly ionized atomic tungsten ions in their 5s25p65d4(5D)6s  6DJ5s^2 5p^6 5d^4({^5}D)6s \; {^6}{\rm D}_{J}, JJ=1/2, ground level and the associated excited metastable levels with JJ=3/2, 5/2, 7/2 and 9/2. Since the ion beams used in the experiments must be expected to contain long-lived excited states also from excited configurations, additional cross-section calculations were performed for the second-lowest term, 5d5  6SJ5d^5 \; ^6{\rm S}_{J}, JJ=5/2, and for the 4^4F term, 5d36s2  4FJ5d^3 6s^2 \; ^4{\rm F}_{J}, with JJ = 3/2, 5/2, 7/2 and 9/2. Given the complexity of the electronic structure of W+^+ the calculations reproduce the main features of the experimental cross section quite well.Comment: 23 pages, 7 figures, 1 table: Accepted for publication in J. Phys. B: At. Mol. & Opt. Phy

    Photoionization of tungsten ions: experiment and theory for W4+^{4+}

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    Experimental and theoretical results are reported for single-photon single ionization of the tungsten ion W4+^{4+}. Absolute cross sections have been measured employing the photon-ion merged-beams setup at the Advanced Light Source in Berkeley. Detailed photon-energy scans were performed at 200~meV bandwidth in the 40 -- 105~eV range. Theoretical results have been obtained from a Dirac-Coulomb R-matrix approach employing basis sets of 730 levels for the photoionization of W4+^{4+}. Calculations were carried out for the 4f145s25p65d2  3FJ4f^{14}5s^2 5p^6 5d^2 \; {^3}{\rm F}_{J}, JJ=2, ground level and the associated fine-structure levels with JJ=3 and 4 for the W4+^{4+} ions. In addition, cross sections have been calculated for the metastable levels 4f145s25p65d2  3P0,1,2,1D2,1G4,1S04f^{14}5s^2 5p^6 5d^2 \; {^3}{\rm P}_{0,1,2},{^1}{\rm D}_{2},{^1}{\rm G}_{4},{^1}{\rm S}_{0}. Very satisfying agreement of theory and experiment is found for the photoionization cross section of W4+^{4+} which is remarkable given the complexity of the electronic structure of tungsten ions in low charge states.Comment: 15 pages, 3 figures, to appear in the Journal of Physics B: Atomic, Molecular and Optical Physic

    New Atomic Data for Trans-Iron Elements and Their Application to Abundance Determinations in Planetary Nebulae

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    [Abridged] Investigations of neutron(n)-capture element nucleosynthesis and chemical evolution have largely been based on stellar spectroscopy. However, the recent detection of these elements in several planetary nebulae (PNe) indicates that nebular spectroscopy is a promising new tool for such studies. In PNe, n-capture element abundance determinations reveal details of s-process nucleosynthesis and convective mixing in evolved low-mass stars, as well as the chemical evolution of elements that cannot be detected in stellar spectra. Only one or two ions of a given trans-iron element can typically be detected in individual nebulae. Elemental abundance determinations thus require corrections for the abundances of unobserved ions. Such corrections rely on the availability of atomic data for processes that control the ionization equilibrium of nebulae. Until recently, these data were unknown for virtually all n-capture element ions. For the first five ions of Se, Kr, and Xe -- the three most widely detected n-capture elements in PNe -- we are calculating photoionization cross sections and radiative and dielectronic recombination rate coefficients using the multi-configuration Breit-Pauli atomic structure code AUTOSTRUCTURE. Charge transfer rate coefficients are being determined with a multichannel Landau-Zener code. To calibrate these calculations, we have measured absolute photoionization cross sections of Se and Xe ions at the Advanced Light Source synchrotron radiation facility. These atomic data can be incorporated into photoionization codes, which we will use to derive ionization corrections (hence abundances) for Se, Kr, and Xe in ionized nebulae. These results are critical for honing nebular spectroscopy into a more effective tool for investigating the production and chemical evolution of trans-iron elements in the Universe.Comment: 10 pages, 2 figures, accepted for publication in the Canadian Journal of Physic

    State-resolved valence shell photoionization of Be-like ions: experiment and theory

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    High-resolution photoionization experiments were carried out using beams of Be-like C2+^{2+}, N3+^{3+}, and O4+^{4+} ions with roughly equal populations of the 1^1S ground-state and the 3^3Po^o manifold of metastable components. The energy scales of the experiments are calibrated with uncertainties of 1 to 10 meV depending on photon energy. Resolving powers beyond 20,000 were reached allowing for the separation of contributions from the individual metastable 3^3P0o^o_0, 3^3P1o^o_1, and 3^3P2o^o_2 states. The measured data compare favourably with semi-relativistic Breit-Pauli R-matrixComment: 23 figures and 3 table

    Interplay of the volume and surface plasmons in the electron energy loss spectra of C60_{60}

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    The results of a joint experimental and theoretical investigation of the C60 collective excitations in the process of inelastic scattering of electrons are presented. The shape of the electron energy loss spectrum is observed to vary when the scattering angle increases. This variation arising due to the electron diffraction of the fullerene shell is described by a new theoretical model which treats the fullerene as a spherical shell of a finite width and accounts for the two modes of the surface plasmon and for the volume plasmon as well. It is shown that at small angles, the inelastic scattering cross section is determined mostly by the symmetric mode of the surface plasmon, while at larger angles, the contributions of the antisymmetric surface plasmon and the volume plasmon become prominent.Comment: 11 pages, 3 figure

    Photoionization of the fullerene ion C60+

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    Photoionization cross section of the fullerene ion C60+ has been calculated within a single-electron approximation and also by using a consistent many-body theory accounting for many-electron correlations.Comment: 8 pages, 3 figure
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