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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.73.205121
|2 DOI
024 7 _ |a WOS:000237950500028
|2 WOS
024 7 _ |a 2128/1445
|2 Handle
037 _ _ |a PreJuSER-52189
041 _ _ |a eng
082 _ _ |a 530
084 _ _ |2 WoS
|a Physics, Condensed Matter
100 1 _ |a Sangiovanni, G.
|b 0
|0 P:(DE-HGF)0
245 _ _ |a Static versus dynamical mean-field theory of Mott antiferromagnets
260 _ _ |a College Park, Md.
|b APS
|c 2006
300 _ _ |a 205121
336 7 _ |a Journal Article
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336 7 _ |a article
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440 _ 0 |a Physical Review B
|x 1098-0121
|0 4919
|v 73
500 _ _ |a Record converted from VDB: 12.11.2012
520 _ _ |a Studying the antiferromagnetic phase of the Hubbard model by dynamical mean-field theory, we observe striking differences with static (Hartree-Fock) mean field: The Slater band is strongly renormalized and spectral weight is transferred to spin-polaron sidebands. Already for intermediate values of the interaction U the overall bandwidth is larger than in the Hartree-Fock mean field and the gap is considerably smaller. Such differences survive any renormalization of U. Our photoemission experiments for Cr-doped V2O3 show spectra qualitatively well described by dynamical mean-field theory.
536 _ _ |a Kondensierte Materie
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542 _ _ |i 2006-05-31
|2 Crossref
|u http://link.aps.org/licenses/aps-default-license
588 _ _ |a Dataset connected to Web of Science
650 _ 7 |a J
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700 1 _ |a Toschi, A.
|b 1
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700 1 _ |a Koch, E.
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|u FZJ
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700 1 _ |a Held, K.
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700 1 _ |a Capone, M.
|b 4
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700 1 _ |a Castellani, C.
|b 5
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700 1 _ |a Gunnarsson, O.
|b 6
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700 1 _ |a Mo, S.-K.
|b 7
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700 1 _ |a Allen, J. W.
|b 8
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700 1 _ |a Kim, H.-D.
|b 9
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700 1 _ |a Sekiyama, A.
|b 10
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700 1 _ |a Yamasaki, A.
|b 11
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700 1 _ |a Suga, S.
|b 12
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700 1 _ |a Metcalf, P.
|b 13
|0 P:(DE-HGF)0
773 1 8 |a 10.1103/physrevb.73.205121
|b American Physical Society (APS)
|d 2006-05-31
|n 20
|p 205121
|3 journal-article
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|t Physical Review B
|v 73
|y 2006
|x 1098-0121
773 _ _ |a 10.1103/PhysRevB.73.205121
|g Vol. 73, p. 205121
|p 205121
|n 20
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|0 PERI:(DE-600)2844160-6
|t Physical review / B
|v 73
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856 7 _ |u http://dx.doi.org/10.1103/PhysRevB.73.205121
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856 4 _ |u https://juser.fz-juelich.de/record/52189/files/82047.pdf
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999 C 5 |a 10.1103/PhysRev.140.A1133
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999 C 5 |a 10.1103/RevModPhys.61.689
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999 C 5 |a 10.1103/PhysRevB.44.943
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999 C 5 |a 10.1088/0953-8984/9/4/002
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999 C 5 |a 10.1088/0953-8984/9/35/010
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999 C 5 |a 10.1103/PhysRevB.57.6884
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999 C 5 |a 10.1103/PhysRevLett.62.324
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999 C 5 |a 10.1103/RevModPhys.68.13
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999 C 5 |a 10.1103/PhysRevLett.69.168
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999 C 5 |a 10.1103/PhysRevLett.80.2393
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999 C 5 |a 10.1140/epjb/e2002-00180-3
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999 C 5 |a 10.1088/0953-8984/15/46/006
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999 C 5 |a 10.1103/PhysRevB.46.13852
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999 C 5 |a 10.1103/PhysRevLett.72.2761
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999 C 5 |a 10.1103/PhysRevB.2.1324
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|2 Crossref
999 C 5 |1 L. N. Bulaevskii
|y 1968
|2 Crossref
|o L. N. Bulaevskii 1968
999 C 5 |1 L. N. Bulaevskii
|y 1968
|2 Crossref
|o L. N. Bulaevskii 1968
999 C 5 |a 10.1103/PhysRevB.41.2017
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999 C 5 |a 10.1103/PhysRevB.44.317
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999 C 5 |a 10.1103/PhysRevB.66.165102
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999 C 5 |a 10.1103/PhysRevB.51.8337
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999 C 5 |a 10.1007/978-1-4612-0869-3
|1 A. Auerbach
|2 Crossref
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|y 1994
999 C 5 |a 10.1016/S0038-1098(02)00425-8
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999 C 5 |a 10.1143/JPSJ.74.34
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999 C 5 |a 10.1103/PhysRevLett.93.076404
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999 C 5 |a 10.1103/PhysRevB.45.2237
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999 C 5 |a 10.1103/PhysRevLett.86.5345
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999 C 5 |a 10.1103/PhysRevB.70.205116
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|2 Crossref


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