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The previously proposed model postulating that the incommensurately modulated KNd(MoO) structure can act as a generator of the scheelite family members is validated here by refining the crystal structure of europium molybdate, Eu(MoO). The initial structural model was derived from the superspace characteristics of KNd(MoO) and the predicted parameters used in the simulation of Eu(WO). The refinement was performed using both superspace and traditional supercell approaches in superspace group $I2/b(\alpha\beta 0)00 and space group A2/a, respectively. The results obtained by both approaches are in excellent agreement and coincide with those reported in the literature.
Nicola Marzari, Marnik Bercx, Carl Simon Adorf