Photoelectron spectroscopic studies of polyatomic molecules: Spin-polarized electrons from point symmetry group molecules
N. Chandra
Phys. Rev. A 40, 768 (1989) - Published 1 July, 1989
This paper presents a study of angle- and spin-resolved photoelectron spectroscopy in a randomly oriented nonlinear molecule in the nonrelativistic, electric dipole approximation. The theory formulated in the preceding paper has been used along with the methods of the extended point (or spin-double) group to develop, perhaps in their simplest possible forms, the expressions for the five parameters needed to specify the angular distribution of spin-polarized electrons ejected in photoionization by unpolarized, or by linearly or circularly polarized light in the orbital of a molecule. The polarization of the photoelectrons in this case is due directly to the spin-orbit interaction in molecular continua. Such angle- and spin-resolved studies will therefore provide more stringent tests of theoretical models, probes of photoionization dynamics, and a measure of the influence of the spin-orbit interaction on the continuum part of the spectrum.
The procedure adopted and the formulation presented here set a methodology and a framework for the analysis of measurements and calculations of spin-resolved spectra in nonlinear systems in general and molecules in particular. The specific examples treated in this paper are those of photoionization in the respective 4, 6, and 7 orbitals of unoriented , , and molecular targets. Without any dynamical calculations, and by use instead of the experimentally measured values of the angular asymmetry (β¯) as a function of the photon wavelength, the variations in ξ¯, δ¯-γ¯, and 2γ¯+δ¯ with respect to the energy of the incident radiation and to the phases involved have been studied in detail. These three quantities (where γ¯, δ¯, and ξ¯ are the spin parameters) determine the degree of spin polarization of photoelectrons in various experimental configurations. While δ¯-γ¯ is found to be independent of phase, both ξ¯ and 2γ¯+δ¯ depend very strongly upon it. The phase, in turn, is influenced by the spin-orbit interaction. This study has helped also in analyzing and revealing the nature of the Cooper minima observed in (6 and (7 spectra and in predicting the values of the spin parameters γ¯, δ¯, and ξ¯ in the corresponding energy regions.