Energy levels and transition probabilities for Fe xxv ions

The energy levels of the 1s(2), 1s2l and 1s3l states of helium-like iron Fe XXV have been calculated using two sets of configuration-interaction wavef unctions. One set of wavefunctions was generated using the fully relativist ic GRASP code and the other was obtained using CIV3, in which relativistic effects are introduced using the Breit-Pauli approximation. For transitions from the ground state to the n = 2 and 3 states and for transitions betwee n the ii = 2 and 3 states, the calculated excitation energies obtained by t hese two independent methods are in very good agreement and then is good ag reement between these results and recent theoretical and experimental resul ts. However, there is considerable disagreement between the various excitat ion energies for the transitions among the n = 2 and also among the n = 3 s tates. The two sets of wavefunctions are also used to calculate the E1, E2, M1 and M2 transition probabilities between all of the 1s(2), 1s2l and 1s3l states of helium-like iron Fe XXV. The results from the two calculations a re found to be similar and to compare very well with other recent results f or Delta n = 1 or 2 transitions. For Delta n = 0 transitions the agreement is much less satisfactory; this is mainly due to differences in the excitat ion energies.