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Ab initio investigations of magnetic properties of ultrathin transition ...

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56 4 Collinear magnetism <strong>of</strong> 3d-monolayers on Rh substrates<br />

Δd 12 [%]<br />

Δd 23 [%]<br />

−2<br />

−4<br />

−6<br />

−8<br />

−10<br />

−12<br />

8<br />

6<br />

4<br />

2<br />

0<br />

−2<br />

(a)<br />

(b)<br />

FM<br />

AFM<br />

FM<br />

AFM<br />

V Cr Mn Fe Co Ni<br />

Figure 4.4: Relaxations <strong>of</strong> the first and second interlayer spacing, Δd12 (circles) and Δd23<br />

(squares), respectively, for 3d TM monolayers on Rh(001) for the FM (solid symbols connected<br />

by solid lines) and the c(2 × 2) AFM (open symbols connected by dashed line)<br />

configuration. The corresponding changes are given with respect to the substrates bulk<br />

interlayer spacing, which is 1.91 ˚A.<br />

the importance <strong>of</strong> multilayer relaxations for the early <strong>transition</strong> monolayers. The same<br />

trend can be seen for the monolayers with c(2 × 2) AFM configuration: while Δd12 is also<br />

influenced by the <strong>magnetic</strong> moment <strong>of</strong> the 3d monolayer, Δd23 depends almost solely on<br />

the d-band filling.<br />

In Fig. 4.5 the <strong>magnetic</strong> moments <strong>of</strong> the 3d TM monolayers on Rh(001) are compared<br />

with the Ag(001) and Pd(001) substrates for the FM and AFM structures at the relaxed<br />

interlayer distances. The <strong>magnetic</strong> moments for on Rh(001) are smaller than those on<br />

Ag(001) or Pd(001) for the early TMs, while they are quite similar for the late TMs. This<br />

can be understood on the basis <strong>of</strong> the observation, that the overlap <strong>of</strong> the d-wavefunctions<br />

with the substrate is larger for the early than for the late TMs. Therefore, the dependence<br />

<strong>of</strong> the TMs <strong>magnetic</strong> moments on the chosen substrate is largest at the beginning <strong>of</strong> the<br />

TM series. The largest moment, in all cases, is found for Mn. The V and Ni <strong>magnetic</strong><br />

moments vanish for the c(2 × 2) AFM structure. The induced <strong>magnetic</strong> moment <strong>of</strong> the<br />

Rh interface layer couples antiferro<strong>magnetic</strong>ally with Cr and ferro<strong>magnetic</strong>ally with Mn,<br />

Fe, Co and Ni, while almost no moment is induced by V. The largest induced <strong>magnetic</strong><br />

moment is caused by the Co monolayer. The induced moments are much larger for Rh<br />

than for substrates like Ag(001), highlighting the importance <strong>of</strong> the substrate for <strong>magnetic</strong><br />

<strong>properties</strong> like the magnetocrystalline anisotropy (MCA), which will be discussed later. Of<br />

course the AFM ordered TM films induce no <strong>magnetic</strong> moment in the interface Rh layer,<br />

and the induced moments in the deeper layers are considerably smaller (and <strong>of</strong> opposite<br />

orientation).

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