572 research outputs found
Single-photon single ionization of W ions: experiment and theory
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 , =1/2, ground level and the associated
excited metastable levels with =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, , =5/2, and for
the F term, , with = 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 W
Experimental and theoretical results are reported for single-photon single
ionization of the tungsten ion W. 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 W. Calculations were carried out for the
, =2, ground level and the
associated fine-structure levels with =3 and 4 for the W ions. In
addition, cross sections have been calculated for the metastable levels
. Very satisfying agreement of theory and experiment is
found for the photoionization cross section of W 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
[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
High-resolution photoionization experiments were carried out using beams of
Be-like C, N, and O ions with roughly equal populations of
the S ground-state and the P 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
P, P, and P 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 C
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+
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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