Recent in situ polarized neutron-reflectometry and magneto-optical Kerr eff
ect measurements have displayed a few magnetically dead Fe layers deposited
on V(110). We have performed ab initio density-functional theory calculati
ons in order to explain the a priori unexpected results. An ideal layer-by-
layer growth of Fe on the V(110) surface leads to the ferromagnetic solutio
n for every Fe thickness. However, if alloying is present at the interface,
a strong decrease in the Fe magnetization is found. We discuss the differe
nt magnetic configurations and the possible mechanisms that can produce the
observed magnetically dead Fe layers.