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

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Summary and conclusions<br />

As a conclusion <strong>of</strong> this thesis, we employed the full-potential linearized augmented planewave<br />

(FLAPW) method to report a systematic density-functional (DFT) study <strong>of</strong> the<br />

<strong>magnetic</strong> <strong>properties</strong> <strong>of</strong> the 3d <strong>transition</strong>-metal (V, Cr, Mn, Fe, Co and Ni) monolayers<br />

deposited on the Rh(001) and Rh(111) substrates. In order to get a better understanding <strong>of</strong><br />

the <strong>magnetic</strong> phases which could become realistically possible we have mapped in part the<br />

ab <strong>initio</strong> result onto model Hamiltonians, predominantly the Heisenberg model. In some<br />

instances the model was amended by a local term describing the Stoner enhanced <strong>magnetic</strong><br />

polarization <strong>of</strong> the substrate. From the values and sign <strong>of</strong> the intersite exchange interaction<br />

we have drawn conclusions on the possible <strong>magnetic</strong> structure. For Fe on Rh(111) we<br />

predicted a novel <strong>magnetic</strong> phase, a double-row-wise antiferro<strong>magnetic</strong> (double-row-AFM)<br />

structure along the [112] direction.<br />

At first we scanned the <strong>magnetic</strong> phase space by restricting ourselves to collinear <strong>magnetic</strong><br />

states, the results <strong>of</strong> which are outlined in Chapter 4. Performing collinear calculations<br />

for the ferro<strong>magnetic</strong> (FM) and antiferro<strong>magnetic</strong> (AFM) state, we relaxed our<br />

structures using atomic force calculations, and compared the relaxations between both<br />

states on both Rh surfaces. We found, all monolayer films are <strong>magnetic</strong>. The size <strong>of</strong> the<br />

local <strong>magnetic</strong> moments across the <strong>transition</strong>-metal series follows Hund’s rule with a maximum<br />

<strong>magnetic</strong> moment <strong>of</strong> 3.77 μB for Mn. The largest induced <strong>magnetic</strong> moment <strong>of</strong> about<br />

0.46 μB was found for Rh atoms adjacent to the Co-film on Rh(001). When relaxations<br />

are included, we predict a ferro<strong>magnetic</strong> ground state for V, Co and Ni, while Cr, Mn and<br />

Fe deposited on the Rh(001) substrate favor a c(2 × 2) antiferro<strong>magnetic</strong> state, a checkerboard<br />

arrangement <strong>of</strong> up and down <strong>magnetic</strong> moments. To gain an understanding <strong>of</strong> the<br />

c(2 × 2) AFM state <strong>of</strong> Fe/Rh(001), we analyzed this result with respect to the trends <strong>of</strong><br />

the <strong>magnetic</strong> order <strong>of</strong> 3d monolayers on other 4d substrates, such as Pd(001) and Ag(001).<br />

The <strong>magnetic</strong> anisotropy energies <strong>of</strong> these <strong>ultrathin</strong> <strong>magnetic</strong> films on the Rh(001) are<br />

calculated for the FM and the AFM states. With the exception <strong>of</strong> V and Cr, the easy axis<br />

<strong>of</strong> the magnetization is predicted to be in the film plane. The Rh(111) substrate did not<br />

change the <strong>magnetic</strong> ground state except for Fe, where it changed from AFM on Rh(001)<br />

to FM on Rh(111). This change deserved a more detailed analysis which is presented in<br />

Chapter 5.<br />

The FM ground state <strong>of</strong> Fe monolayer on Rh(111) could not be explained from the<br />

non<strong>magnetic</strong> density <strong>of</strong> states and the Stoner model. Total-energy calculations show that<br />

the energy difference to the AFM state is rather small and the <strong>magnetic</strong> structure might be<br />

115

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