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

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86 5 Fe monolayers on hexagonal non<strong>magnetic</strong> substrates<br />

structures the Mn 3d-band filling is increased. This supports our idea that the exchange<br />

interaction parameters can be controlled by tuning the substrate, which might lead to<br />

unexpected complex <strong>magnetic</strong> structures.<br />

5.2.2 Results <strong>of</strong> Fe monolayer on Rh(111):<br />

In this section, the search for the <strong>magnetic</strong> ground state <strong>of</strong> Fe on Rh and Tc will be shown<br />

by performing non-collinear spin-spiral calculations along the high symmetry line, Γ-K-M-<br />

Γ, in the hexagonal BZ. The non-collinear <strong>magnetic</strong> states have been studied employing an<br />

asymmetric film consisting <strong>of</strong> six substrate layers and an Fe monolayer on one side <strong>of</strong> the<br />

film at the distance optimized for the collinear (FM or AFM) state <strong>of</strong> lowest energy. The<br />

spin spirals have been calculated exploiting the generalized Bloch theorem [83]. We have<br />

used about 120 basis functions per atom for all calculations and at least 1024 k� points in<br />

the 2D-BZ for the spin-spiral calculations, 48 k� points in one quarter <strong>of</strong> the 2D-BZ for<br />

the uudd configurations and 32 k� points in the 2D-BZ for the 3Q-state requiring a surface<br />

unit-cell comprising 4 atoms. All other numerical parameters were kept to be the same as<br />

for the collinear calculations in sec. (4.3.1).<br />

The total energy relative to the FM spin configuration <strong>of</strong> Fe monolayer on Rh(111), is<br />

shown in fig. 5.7 as a function <strong>of</strong> the spin-spiral q-vector, using GGA and LDA exchange<br />

correlation potentials, along the high symmetry line Γ-K-M-Γ, and for hcp or fcc Fe-Rh(I)<br />

stacking. We see that both stacking sequences share the same global minimum energy. The<br />

fcc Fe-Rh(I) is lower than the hcp stacking minimum energy by ∼−5 meV/Fe atom. But<br />

the Fe prefers hcp stacking by −9 meV/Fe atom (see subsec. 5.1.2) from the independently<br />

FM relaxed solution <strong>of</strong> each stacking, this means that the real spin spiral curve <strong>of</strong> the hcp<br />

Fe-Rh(I) stacking is lower in energy by −9meV, i. e. the hcp is lower than the fcc stacking<br />

global minimum energy by −4 meV/Fe atom, provided that the difference between fcc and<br />

hcp Fe-Rh(I) optimized d12 was 0.01˚A. We checked that, and found the our analogy is true,<br />

the hcp at the minimum q-point is always lower than the fcc stacking total energy by −4<br />

meV/Fe atom. Because <strong>of</strong> that, we always use the Fe-Rh(I) hcp stacking results. On the<br />

other hand, we compare GGA and LDA results, and we see that both confirm the same<br />

result, where Fe monolayer might have a possible spin spiral ground state along Γ-K, with<br />

−5 (−10) meV/Fe atom in case <strong>of</strong> GGA (LDA).<br />

A simple approach to estimate the J’s, is to exclude the higher order terms in equation<br />

A-20, and calculate J1, J2 and J3 from the high symmetry points total energies, Γ, M<br />

and K, where they are presented in terms <strong>of</strong> J1, J2 and J3 from equation A-20 as following:<br />

EΓ = −M2 (6J1 +6J2 +6J3)<br />

EM = −M2 (−2J1 − 2J2 +6J3)<br />

EK = −M2 (−3J1 +6J2− 3J3) (5.15)<br />

As a simple approximation, if the variation <strong>of</strong> Fe <strong>magnetic</strong> moments is considerably small<br />

at the high symmetry points, , we can assume an arbitrary value <strong>of</strong> M=1. We have three

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