Hauptseite > Publikationsdatenbank > Unexpected trend of magnetic order of 3d transition-metal monolayers on W(001) > print |
001 | 46383 | ||
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017 | _ | _ | |a This version is available at the following Publisher URL: http://prb.aps.org |
024 | 7 | _ | |a 10.1103/PhysRevB.72.024452 |2 DOI |
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041 | _ | _ | |a eng |
082 | _ | _ | |a 530 |
084 | _ | _ | |2 WoS |a Physics, Condensed Matter |
100 | 1 | _ | |a Ferriani, P. |b 0 |0 P:(DE-HGF)0 |
245 | _ | _ | |a Unexpected trend of magnetic order of 3d transition-metal monolayers on W(001) |
260 | _ | _ | |a College Park, Md. |b APS |c 2005 |
300 | _ | _ | |a 024452 |
336 | 7 | _ | |a Journal Article |0 PUB:(DE-HGF)16 |2 PUB:(DE-HGF) |
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336 | 7 | _ | |a article |2 DRIVER |
440 | _ | 0 | |a Physical Review B |x 1098-0121 |0 4919 |v 72 |
500 | _ | _ | |a Record converted from VDB: 12.11.2012 |
520 | _ | _ | |a We report systematic first-principles calculations based on the full-potential linearized augmented plane wave method for 3d transition-metal (V, Cr, Mn, Fe, Co, Ni) monolayers on the W(001) surface. We predict that V, Cr, and Mn monolayers exhibit a ferromagnetic ground state, while Fe and Co favor the c(2 x 2) antiferromagnetic state. This trend is surprising as it is opposite to what was expected from the knowledge of magnetism in ultrathin films and results from strong hybridization at the W interface. In particular, this system is the first case showing antiferromagnetic Co. |
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542 | _ | _ | |i 2005-07-25 |2 Crossref |u http://link.aps.org/licenses/aps-default-license |
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700 | 1 | _ | |a Heinze, S. |b 1 |0 P:(DE-HGF)0 |
700 | 1 | _ | |a Bihlmayer, G. |b 2 |u FZJ |0 P:(DE-Juel1)130545 |
700 | 1 | _ | |a Blügel, S. |b 3 |u FZJ |0 P:(DE-Juel1)130548 |
773 | 1 | 8 | |a 10.1103/physrevb.72.024452 |b American Physical Society (APS) |d 2005-07-25 |n 2 |p 024452 |3 journal-article |2 Crossref |t Physical Review B |v 72 |y 2005 |x 1098-0121 |
773 | _ | _ | |a 10.1103/PhysRevB.72.024452 |g Vol. 72, p. 024452 |p 024452 |n 2 |q 72<024452 |0 PERI:(DE-600)2844160-6 |t Physical review / B |v 72 |y 2005 |x 1098-0121 |
856 | 7 | _ | |u http://dx.doi.org/10.1103/PhysRevB.72.024452 |u http://hdl.handle.net/2128/1414 |
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