Frank Larkins - Academia.edu (original) (raw)
Papers by Frank Larkins
Energy & Fuels, 1990
ABSTRACT
J Phys B at Mol Opt Phys, 1994
Journal of Physics B Atomic and Molecular Physics
ABSTRACT
Journal of Physics B Atomic and Molecular Physics
ABSTRACT
Journal of Physics B Atomic and Molecular Physics
ABSTRACT
Coal Science and Technology, 1995
Coal Science and Technology, 1995
Journal of Physics B-atomic Molecular and Optical Physics - J PHYS-B-AT MOL OPT PHYS, 1982
A model for the calculation of satellite structure in atomic spectra is presented. Based on numer... more A model for the calculation of satellite structure in atomic spectra is presented. Based on numerical non-relativistic wavefunctions, it includes some of the effects of electron correlation via frozen-core CI calculations. The model is applied to the energies of the 2S, 2P0 and 2D states of the singly ionised rare gases Ne, Ar, Kr and Xe. The results agree with experiment to within 1 eV for most excitation energies in Ar, Kr and Xe, and for Ne when relaxation of the frozen core is accounted for. Some trends in excitation energies with atomic number are discussed, and the model's performance in the prediction of excitation energies is assessed.
Physical Review A, 1998
Sulfur Kβ x-ray emission from carbonyl sulfide: Variations with polarization and excitation energ... more Sulfur Kβ x-ray emission from carbonyl sulfide: Variations with polarization and excitation energy at the SK threshold. KE Miyano Department of Physics, Brooklyn College, Brooklyn, New York 11210. U. Arp National Institute of ...
Journal of Physics B: Atomic, Molecular and Optical Physics, 1991
ABSTRACT
Information Processing Letters
Journal of Electron Spectroscopy and Related Phenomena, 1995
Carbon K X-ray emission transition energies and probabilities have been calculated for the fluoro... more Carbon K X-ray emission transition energies and probabilities have been calculated for the fluoromethane series of molecules CH4−xFx, where x is 0–4, subsequent to carbon K-shell photoionization. Four methods were used to calculate the transition probabilities: the ground state frozen orbital method, the core-hole frozen orbital method, the transition state method, and the fully relaxed orbital method. The results were
Journal of Physics B: Atomic and Molecular Physics, 1981
ABSTRACT
Journal of Physics B-atomic Molecular and Optical Physics - J PHYS-B-AT MOL OPT PHYS, 1982
for pt.I see ibid., vol.15, p.203 (1982). A model for the calculation of atomic satellite structu... more for pt.I see ibid., vol.15, p.203 (1982). A model for the calculation of atomic satellite structure described in an earlier paper, is applied to the outer-shell photoelectron spectra of the rare gases neon, argon, krypton and xenon using muti-configuration shake theory to calculate relative intensities. The origin of the satellite structure and some trends with atomic number are discussed. The high-energy photon spectra are interpreted, although for Xe the importance of relativistic effects prevents a complete interpretation. The model is found to have achieved its aim of providing both an understanding and a basis for interpretation of atomic satellite spectra.
Journal of Physics B: Atomic and Molecular Physics, 1982
For pt.II see ibid., vol.15, no.2, p.219-31 (1982). The satellite structure in the argon L X-ray ... more For pt.II see ibid., vol.15, no.2, p.219-31 (1982). The satellite structure in the argon L X-ray emission spectrum has been calculated using correlated initial- and final-state wavefunctions based upon a frozen-core model for each state developed previously. Strong correlation effects in the final state give rise to intense satellite structure similar to the photoelectron satellites seen in valence-shell ionisation. The
The Journal of Chemical Physics, 1988
We present here a semiempirical assignment for the electronic decay spectra of core to bound stat... more We present here a semiempirical assignment for the electronic decay spectra of core to bound state resonances in N2O. The electronic final states observed in these spectra can be assigned to participator and spectator decay processes, according to whether the initially excited core electron participates or acts as a spectator in the Auger decay of the core hole. The participator states are interpreted empirically using the known one electron binding energies. The assignment of the spectator lines is derived from the calculated Auger spectrum which is corrected for the Coulomb interaction between the spectator electron and the double hole valence configuration.
Energy & Fuels, 1990
ABSTRACT
J Phys B at Mol Opt Phys, 1994
Journal of Physics B Atomic and Molecular Physics
ABSTRACT
Journal of Physics B Atomic and Molecular Physics
ABSTRACT
Journal of Physics B Atomic and Molecular Physics
ABSTRACT
Coal Science and Technology, 1995
Coal Science and Technology, 1995
Journal of Physics B-atomic Molecular and Optical Physics - J PHYS-B-AT MOL OPT PHYS, 1982
A model for the calculation of satellite structure in atomic spectra is presented. Based on numer... more A model for the calculation of satellite structure in atomic spectra is presented. Based on numerical non-relativistic wavefunctions, it includes some of the effects of electron correlation via frozen-core CI calculations. The model is applied to the energies of the 2S, 2P0 and 2D states of the singly ionised rare gases Ne, Ar, Kr and Xe. The results agree with experiment to within 1 eV for most excitation energies in Ar, Kr and Xe, and for Ne when relaxation of the frozen core is accounted for. Some trends in excitation energies with atomic number are discussed, and the model's performance in the prediction of excitation energies is assessed.
Physical Review A, 1998
Sulfur Kβ x-ray emission from carbonyl sulfide: Variations with polarization and excitation energ... more Sulfur Kβ x-ray emission from carbonyl sulfide: Variations with polarization and excitation energy at the SK threshold. KE Miyano Department of Physics, Brooklyn College, Brooklyn, New York 11210. U. Arp National Institute of ...
Journal of Physics B: Atomic, Molecular and Optical Physics, 1991
ABSTRACT
Information Processing Letters
Journal of Electron Spectroscopy and Related Phenomena, 1995
Carbon K X-ray emission transition energies and probabilities have been calculated for the fluoro... more Carbon K X-ray emission transition energies and probabilities have been calculated for the fluoromethane series of molecules CH4−xFx, where x is 0–4, subsequent to carbon K-shell photoionization. Four methods were used to calculate the transition probabilities: the ground state frozen orbital method, the core-hole frozen orbital method, the transition state method, and the fully relaxed orbital method. The results were
Journal of Physics B: Atomic and Molecular Physics, 1981
ABSTRACT
Journal of Physics B-atomic Molecular and Optical Physics - J PHYS-B-AT MOL OPT PHYS, 1982
for pt.I see ibid., vol.15, p.203 (1982). A model for the calculation of atomic satellite structu... more for pt.I see ibid., vol.15, p.203 (1982). A model for the calculation of atomic satellite structure described in an earlier paper, is applied to the outer-shell photoelectron spectra of the rare gases neon, argon, krypton and xenon using muti-configuration shake theory to calculate relative intensities. The origin of the satellite structure and some trends with atomic number are discussed. The high-energy photon spectra are interpreted, although for Xe the importance of relativistic effects prevents a complete interpretation. The model is found to have achieved its aim of providing both an understanding and a basis for interpretation of atomic satellite spectra.
Journal of Physics B: Atomic and Molecular Physics, 1982
For pt.II see ibid., vol.15, no.2, p.219-31 (1982). The satellite structure in the argon L X-ray ... more For pt.II see ibid., vol.15, no.2, p.219-31 (1982). The satellite structure in the argon L X-ray emission spectrum has been calculated using correlated initial- and final-state wavefunctions based upon a frozen-core model for each state developed previously. Strong correlation effects in the final state give rise to intense satellite structure similar to the photoelectron satellites seen in valence-shell ionisation. The
The Journal of Chemical Physics, 1988
We present here a semiempirical assignment for the electronic decay spectra of core to bound stat... more We present here a semiempirical assignment for the electronic decay spectra of core to bound state resonances in N2O. The electronic final states observed in these spectra can be assigned to participator and spectator decay processes, according to whether the initially excited core electron participates or acts as a spectator in the Auger decay of the core hole. The participator states are interpreted empirically using the known one electron binding energies. The assignment of the spectator lines is derived from the calculated Auger spectrum which is corrected for the Coulomb interaction between the spectator electron and the double hole valence configuration.