001     156098
005     20230426083113.0
024 7 _ |2 doi
|a 10.1103/PhysRevB.90.115427
024 7 _ |2 ISSN
|a 0163-1829
024 7 _ |2 ISSN
|a 1095-3795
024 7 _ |2 ISSN
|a 1550-235X
024 7 _ |2 ISSN
|a 0556-2805
024 7 _ |2 ISSN
|a 1098-0121
024 7 _ |2 WOS
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024 7 _ |2 Handle
|a 2128/9116
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037 _ _ |a FZJ-2014-04972
082 _ _ |a 530
100 1 _ |0 P:(DE-Juel1)131065
|a Zimmermann, Bernd
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245 _ _ |a First-principles analysis of a homochiral cycloidal magnetic structure in a monolayer Cr on W(110)
260 _ _ |a College Park, Md.
|b APS
|c 2014
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520 _ _ |a The magnetic structure of a Cr monolayer on a W(110) substrate is investigated by means of first-principles calculations based on noncollinear spin density functional theory (DFT). As magnetic ground state we find a long-period homochiral left-rotating spin spiral on top of an atomic-scale antiferromagnetic order of nearest-neighbor atoms. The rotation angle of the magnetic moment changes inhomogeneously from atom to atom across the spiral. We predict a propagation direction along the crystallographic [001] direction with a period length of |λ|=14.3nm, which is in excellent agreement with a modulation of the local antiferromagnetic contrast observed in spin-polarized scanning tunneling microscope experiments by Santos et al. [New J. Phys. 10, 013005 (2008)]. We identify the Dzyaloshinskii-Moriya interaction as the origin of the homochiral magnetic structure, competing with the Heisenberg-type exchange interaction and magnetocrystalline anisotropy energy. From DFT calculations we extract parameters for a micromagnetic model and thereby determine a considerable inhomogeneity of the spin spiral, increasing the period length by 6% compared to homogeneous spin spirals. The results are compared to the behavior of a Mn and Fe monolayer and Fe double layer on a W(110) substrate.
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|a Heide, Marcus
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700 1 _ |0 P:(DE-Juel1)130545
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700 1 _ |0 P:(DE-Juel1)130548
|a Blügel, Stefan
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773 1 8 |a 10.1103/physrevb.90.115427
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|t Physical Review B
|v 90
|y 2014
|x 1098-0121
773 _ _ |a 10.1103/PhysRevB.90.115427
|g Vol. 90, no. 11, p. 115427
|0 PERI:(DE-600)2844160-6
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|v 90
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