21.12.2012 Views

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

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

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

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

88 5 Fe monolayers on hexagonal non<strong>magnetic</strong> substrates<br />

below the M, the RW-AFM phase, value using GGA (LDA). Then we calculated B1 and<br />

K1 values using equations (5.8 and 5.14) for the Q 3ΓK/4 and got B1 = −0.6 and K1 =0.0<br />

meV/Fe atom, we then added these values to the model Hamiltonian constructed along<br />

Γ-K-M, and used it to fit our calculated energy dispersion curve to calculate the exchange<br />

interaction parameters, which are shown in table 5.2.<br />

Table 5.2: GGA and LDA results <strong>of</strong> Heisenberg exchange constants for the hcp Fe ML on Rh(111)<br />

substrate obtained by fitting the total-energy dispersion along Γ-K-M and the higher order terms<br />

B1 and K1<br />

(meV) J1 J2 J3 J4 B1 K1<br />

GGA 3.8 −0.6 −1.6 0.3 −0.6 0.0<br />

LDA 3.9 −0.7 −1.1 0.4 −1.3 0.5<br />

We see that GGA and LDA values <strong>of</strong> J1, J2 and J3 are very similar, but different from what<br />

we got when we exclude the higher order interaction terms, using Eq. (5.15). These results<br />

show how important is to include the higher order terms in the model Hamiltonian to get<br />

accurate values <strong>of</strong> the exchange interaction parameters. If we use the values <strong>of</strong> J3/|J1| and<br />

J2/|J1| from the shown results in table 5.2, we find that Fe has non-collinear spin spiral<br />

along Γ-K-M on Rh(111) substrate, but still very close to to FM phase <strong>transition</strong>, referring<br />

to the calculated phase diagrams in figure 5.6. This is consistent with the minimum −5<br />

meV/Fe atom total energy difference below the Γ point, i.e. the FM solution. From the<br />

calculated higher order interactions parameters, we notice that the biquadratic interaction<br />

term B1 is in the same order as the next nearest neighbor term J2, where as the 4-spin<br />

interaction term K1 is zero. In this case we can interpret our results keeping in mind that<br />

if the Fe atoms nearest neighbor interactions are relatively weak compared to next nearest<br />

neighbor interactions, the higher order terms are very important and cannot be ignored<br />

due to their highly possible contribution <strong>of</strong> stabilizing non-collinear ground state.<br />

Because <strong>of</strong> the small ground state total energy difference, the above interpretation is<br />

not a final answer since we are not sure if this small energy difference yields the global<br />

minimum or not, especially since the difference k-points sampling between the spin spiral,<br />

collinear (for double-Q) and the real space (for 3Q) calculations will produce about 5<br />

meV/Fe atom numerical error as it was checked for free-standing Fe monolayer. Because<br />

<strong>of</strong> that, we calculated the total energy <strong>of</strong> the double-Q state along the line M-Γ, which<br />

is constructed by a superposition <strong>of</strong> two Q points at Q MΓ/2 , which represents a collinear<br />

<strong>magnetic</strong> structure in real space called uudd � MΓ/2 � state (see Fig. 5.5). The GGA (LDA)<br />

results show, surprisingly, that the uudd � M Γ/4 � gained about −32 (−27) meV/Fe atom<br />

below the Q M/2 point, and became a global minimum by −30 (−21) meV/Fe atom relative<br />

to FM solution. These results were not expected because uudd � MΓ/2 � and uudd � 3ΓK/4 �<br />

are degenerate according to Heisenberg picture explained in section (3.2), and supposed to<br />

provide the same B1 and K1 values.<br />

Trying to understand the unexpected obtained results for uudd � MΓ/2 � , we plotted the<br />

Fe, the interface layer Rh(I), and the subsurface rhodium layer Rh(I-1) GGA and LDA

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!