“…For Sr Al antisites, only the substitution of Al 3+ by Sr 2+ may be observed for O-poor atmospheres, while all the Sr 0 Al and Sr −1 Al species may appear under O-rich conditions. For the O-intermediate condition, the ε (0/ − 1) charge transition of the Sr Al(1) , Sr Al(2) , Sr Al(4) and Sr Al (5) defects are lying in the lower part of the µ E F allowed range, while the Sr 0 Al(3) and Sr 0 Al(6) species cannot be created. At q = 0, the lowest DFEs are observed for Al(1) sites, i.e.…”