The angular distribution and spin polarisation of the resonantly photoexcited
Xe¤(4d–15/2
6p3/2 )
N5O2,3O2,3
Auger spectrum is investigated. The two-step model has been used which allows
us to independently determine the dynamic parameters of the primary excitation
and the Auger emission process. Assuming either a fully circularly or linearly
polarised photon beam the dynamic parameters determining the primary
photoexcitation become constant numbers independent of the matrix elements.
Applying a relativistic distorted wave approximation the relevant numbers
describing the Auger decay dynamics, i.e. relative intensities, angular
distribution and spin polarisation parameters have been calculated, and are
compared with experimental and other theoretical data. With this, predictions
for the spin polarisation vector are possible. A large degree of dynamic spin
polarisation has been found for all Auger transitions to a final state with
Jf = ½ . This is in
contrast to earlier calculations for diagram Auger transitions. Recently, we
have given an explanation for this deriving propensity rules for resonant
Auger transitions. The propensity rules allow for predictions for which Auger
line a large dynamic spin polarisation can be expected. The predictions are in
accord with our multiconfigurational Dirac–Fock calculations for the
resonant Xe
N5O2,3O2,3
and Ar
L3M2,3M2,3
Auger multiplets. It is demonstrated that the effect of a large spin
polarisation is caused by a large shift of the scattering phase of the emitted
?s1/2 partial waves,
whereas a small spin polarisation is due to a cancellation between the Coulomb
and scattering phases of the partial waves.