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024 7 _ |a 10.1103/PhysRevB.80.081105
|2 DOI
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024 7 _ |a 2128/11033
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037 _ _ |a PreJuSER-5600
041 _ _ |a eng
082 _ _ |a 530
084 _ _ |2 WoS
|a Physics, Condensed Matter
100 1 _ |0 P:(DE-HGF)0
|a Wu, H.
|b 0
245 _ _ |a Spin and orbital states in La1.5 Sr0.5 CoO4 studied by electronic structure calculations
260 _ _ |a College Park, Md.
|b APS
|c 2009
300 _ _ |a 081105
336 7 _ |a Journal Article
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440 _ 0 |0 4919
|a Physical Review B
|v 80
|x 1098-0121
|y 8
500 _ _ |a This work was supported by the Deutsche Forschungsgemeinschaft through SFB 608.
520 _ _ |a Electronic structure of the layered perovskite La1.5Sr0.5CoO4 with a checkerboard Co2+/Co3+ charge order is studied, using the local-spin-density approximation plus Hubbard U calculations including also the spin-orbit coupling and multiplet effect. Our results show that the Co2+ ion is in a high spin state (HS, t(2g)(5)e(g)(2)) and Co3+ low spin state (LS, t(2g)(6)). Due to a small Co2+ t(2g) crystal field splitting, the spin-orbit interaction produces an orbital moment of 0.26 mu(B) and accounts for the observed easy in-plane magnetism. Moreover, we find that the Co3+ intermediate spin state (IS, t(2g)(5)e(g)(1)) has a multiplet splitting of several tenths of eV and the lowest-lying one is still higher than the LS ground state by 120 meV, and that the Co3+ HS state (t(2g)(4)e(g)(2)) is more unstable by 310 meV. Either the IS or HS Co3+ ions would give rise to a wrong magnetic order and anisotropy.
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542 _ _ |i 2009-08-26
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653 2 0 |2 Author
|a band structure
653 2 0 |2 Author
|a density functional theory
653 2 0 |2 Author
|a ground states
653 2 0 |2 Author
|a Hubbard model
653 2 0 |2 Author
|a lanthanum compounds
653 2 0 |2 Author
|a magnetic anisotropy
653 2 0 |2 Author
|a spin-orbit interactions
653 2 0 |2 Author
|a strontium compounds
700 1 _ |0 P:(DE-Juel1)130579
|a Burnus, T.
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773 1 8 |a 10.1103/physrevb.80.081105
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|t Physical Review B
|v 80
|y 2009
|x 1098-0121
773 _ _ |a 10.1103/PhysRevB.80.081105
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|t Physical review / B
|v 80
|y 2009
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856 7 _ |u http://dx.doi.org/10.1103/PhysRevB.80.081105
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