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Physical Review B - Condensed Matter and Materials Physics

Volumn 81, Issue 18, 2010, Pages

Orbital-weight redistribution triggered by spin order in the pnictides

(6) Daghofer, M a Luo, Q L b,c Yu, R d Yao, D X b,c,e Moreo, A b,c Dagotto, E b,c

a IFW DRESDEN (Germany)

b UNIVERSITY OF TENNESSEE (United States)

c OAK RIDGE NATIONAL LABORATORY (United States)

d RICE UNIVERSITY (United States)

e SUN YAT SEN UNIVERSITY (China)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 77955456273 PISSN: 10980121 EISSN: 1550235X Source Type: Journal
DOI: 10.1103/PhysRevB.81.180514 Document Type: Article

Times cited : (64)

References (32)

1
- 33846417321
- 10.1103/PhysRevB.75.035110;
- S. Lebègue, Phys. Rev. B 75, 035110 (2007) 10.1103/PhysRevB.75. 035110
- (2007) Phys. Rev. B , vol.75 , pp. 035110
- Lebègue, S.¹

2
- 45249110406
- 10.1103/PhysRevLett.100.237003;
- D. J. Singh and M.-H. Du, Phys. Rev. Lett. 100, 237003 (2008) 10.1103/PhysRevLett.100.237003
- (2008) Phys. Rev. Lett. , vol.100 , pp. 237003
- Singh, D.J.¹ Du, M.-H.²

3
- 79051469407
- 10.1209/0295-5075/82/67002;
- G. Xu, EPL 82, 67002 (2008) 10.1209/0295-5075/82/67002
- (2008) EPL , vol.82 , pp. 67002
- Xu, G.¹

4
- 45749121932
- 10.1103/PhysRevB.77.220506;
- C. Cao, P. J. Hirschfeld, and H.-P. Cheng, Phys. Rev. B 77, 220506 (R) (2008) 10.1103/PhysRevB.77.220506
- (2008) Phys. Rev. B , vol.77 , pp. 220506
- Cao, C.¹ Hirschfeld, P.J.² Cheng, H.-P.³

5
- 66149108052
- 10.1088/0256-307X/26/1/017401;
- H.-J. Zhang, G. Xu, X. Dai, and Z. Fang, Chin. Phys. Lett. 26, 017401 (2009) 10.1088/0256-307X/26/1/017401
- (2009) Chin. Phys. Lett. , vol.26 , pp. 017401
- Zhang, H.-J.¹ Xu, G.² Dai, X.³ Fang, Z.⁴

6
- 47049098637
- 10.1103/PhysRevLett.101.026403
- L. Boeri, O. V. Dolgov, and A. A. Golubov, Phys. Rev. Lett. 101, 026403 (2008). 10.1103/PhysRevLett.101.026403
- (2008) Phys. Rev. Lett. , vol.101 , pp. 026403
- Boeri, L.¹ Dolgov, O.V.² Golubov, A.A.³

7
- 79051469120
- 10.1209/0295-5075/83/27006;
- J. Dong, EPL 83, 27006 (2008) 10.1209/0295-5075/83/27006
- (2008) EPL , vol.83 , pp. 27006
- Dong, J.¹

8
- 45149109919
- 10.1038/nature07057;
- C. de la Cruz, Nature (London) 453, 899 (2008) 10.1038/nature07057
- (2008) Nature (London) , vol.453 , pp. 899
- De La Cruz, C.¹

9
- 50449102951
- 10.1103/PhysRevB.78.064515
- Y. Chen, J. W. Lynn, J. Li, G. Li, G. F. Chen, J. L. Luo, N. L. Wang, P. Dai, C. de la Cruz, and H. A. Mook, Phys. Rev. B 78, 064515 (2008). 10.1103/PhysRevB.78.064515
- (2008) Phys. Rev. B , vol.78 , pp. 064515
- Chen, Y.¹ Lynn, J.W.² Li, J.³ Li, G.⁴ Chen, G.F.⁵ Luo, J.L.⁶ Wang, N.L.⁷ Dai, P.⁸ De La Cruz, C.⁹ Mook, H.A.¹⁰

10
- 74249101533
- 10.1126/science.1181083
- T. Chuang, Science 327, 181 (2010). 10.1126/science.1181083
- (2010) Science , vol.327 , pp. 181
- Chuang, T.¹

11
- 77955455971
- arXiv:1002.3364 (unpublished)
- J. Chu, J. Analytis, K. De Greve, P. McMahon, Z. Islam, Y. Yamamoto, and I. R. Fisher, arXiv:1002.3364 (unpublished).
- Chu, J.¹ Analytis, J.² De Greve, K.³ McMahon, P.⁴ Islam, Z.⁵ Yamamoto, Y.⁶ Fisher, I.R.⁷

12
- 61549126319
- 10.1103/PhysRevB.79.054504
- F. Krüger, S. Kumar, J. Zaanen, and J. van den Brink, Phys. Rev. B 79, 054504 (2009). 10.1103/PhysRevB.79.054504
- (2009) Phys. Rev. B , vol.79 , pp. 054504
- Krüger, F.¹ Kumar, S.² Zaanen, J.³ Van Den Brink, J.⁴

13
- 77955455793
- arXiv:1002.3165 (unpublished)
- W. Lv, F. Krüger, and P. Phillips, arXiv:1002.3165 (unpublished).
- Lv, W.¹ Krüger, F.² Phillips, P.³

14
- 72949104542
- 10.1103/PhysRevLett.103.267001
- C.-C. Lee, W.-G. Yin, and W. Ku, Phys. Rev. Lett. 103, 267001 (2009). 10.1103/PhysRevLett.103.267001
- (2009) Phys. Rev. Lett. , vol.103 , pp. 267001
- Lee, C.-C.¹ Yin, W.-G.² Ku, W.³

15
- 77954793952
- 10.1103/PhysRevB.81.014511
- M. Daghofer, A. Nicholson, A. Moreo, and E. Dagotto, Phys. Rev. B 81, 014511 (2010). 10.1103/PhysRevB.81.014511
- (2010) Phys. Rev. B , vol.81 , pp. 014511
- Daghofer, M.¹ Nicholson, A.² Moreo, A.³ Dagotto, E.⁴

16
- 54849435537
- 10.1103/PhysRevLett.101.167203
- J. Zhao, Phys. Rev. Lett. 101, 167203 (2008). 10.1103/PhysRevLett.101. 167203
- (2008) Phys. Rev. Lett. , vol.101 , pp. 167203
- Zhao, J.¹

17
- 51349156213
- 10.1038/nature07263
- D. H. Lu, Nature (London) 455, 81 (2008). 10.1038/nature07263
- (2008) Nature (London) , vol.455 , pp. 81
- Lu, D.H.¹

18
- 73049099005
- 10.1103/PhysRevB.80.174510
- M. Yi, Phys. Rev. B 80, 174510 (2009). 10.1103/PhysRevB.80.174510
- (2009) Phys. Rev. B , vol.80 , pp. 174510
- Yi, M.¹

19
- 63249112139
- 10.1103/PhysRevB.79.104510
- R. Yu, K. T. Trinh, A. Moreo, M. Daghofer, J. A. Riera, S. Haas, and E. Dagotto, Phys. Rev. B 79, 104510 (2009). 10.1103/PhysRevB.79.104510
- (2009) Phys. Rev. B , vol.79 , pp. 104510
- Yu, R.¹ Trinh, K.T.² Moreo, A.³ Daghofer, M.⁴ Riera, J.A.⁵ Haas, S.⁶ Dagotto, E.⁷

20
- 57349087222
- 10.1103/PhysRevLett.101.237004
- M. Daghofer, A. Moreo, J. A. Riera, E. Arrigoni, D. J. Scalapino, and E. Dagotto, Phys. Rev. Lett. 101, 237004 (2008). 10.1103/PhysRevLett.101.237004
- (2008) Phys. Rev. Lett. , vol.101 , pp. 237004
- Daghofer, M.¹ Moreo, A.² Riera, J.A.³ Arrigoni, E.⁴ Scalapino, D.J.⁵ Dagotto, E.⁶

21
- 59049087890
- 10.1038/nature07714
- V. B. Zabolotnyy, Nature (London) 457, 569 (2009). 10.1038/nature07714
- (2009) Nature (London) , vol.457 , pp. 569
- Zabolotnyy, V.B.¹

22
- 76249123969
- 10.1103/PhysRevLett.104.057002
- T. Shimojima, Phys. Rev. Lett. 104, 057002 (2010). 10.1103/PhysRevLett. 104.057002
- (2010) Phys. Rev. Lett. , vol.104 , pp. 057002
- Shimojima, T.¹

23
- 63449108964
- 10.1088/1367-2630/11/2/025016
- S. Graser, T. A. Maier, P. J. Hirschfeld, and D. J. Scalapino, New J. Phys. 11, 025016 (2009). 10.1088/1367-2630/11/2/025016
- (2009) New J. Phys. , vol.11 , pp. 025016
- Graser, S.¹ Maier, T.A.² Hirschfeld, P.J.³ Scalapino, D.J.⁴

24
- 72049122150
- 10.1103/PhysRevLett.103.247202
- E. Kaneshita, T. Morinari, and T. Tohyama, Phys. Rev. Lett. 103, 247202 (2009). 10.1103/PhysRevLett.103.247202
- (2009) Phys. Rev. Lett. , vol.103 , pp. 247202
- Kaneshita, E.¹ Morinari, T.² Tohyama, T.³

25
- 0001374756
- 10.1103/PhysRevB.28.327
- A. M. Oleś, Phys. Rev. B 28, 327 (1983). 10.1103/PhysRevB.28.327
- (1983) Phys. Rev. B , vol.28 , pp. 327
- Oleś, A.M.¹

26
- 0348107276
- 10.1103/PhysRevLett.91.206402
- M. Potthoff, M. Aichhorn, and C. Dahnken, Phys. Rev. Lett. 91, 206402 (2003). 10.1103/PhysRevLett.91.206402
- (2003) Phys. Rev. Lett. , vol.91 , pp. 206402
- Potthoff, M.¹ Aichhorn, M.² Dahnken, C.³

27
- 77955435683
- Not only is the intraorbital hopping in the x direction smaller for yz than for xz but also the substantial interorbital hopping connecting the yz (xz ) orbitals to xy is 0 along x (y) for symmetry reasons (Ref.)
- Not only is the intraorbital hopping in the x direction smaller for y z than for x z but also the substantial interorbital hopping connecting the y z (x z) orbitals to x y is 0 along x (y) for symmetry reasons (Ref.).

28
- 77955449703
- Since our mean-field approach breaks the orbital symmetry by neglecting the "pair-hopping" and spin-flip terms of the onsite interaction, we have to check that the yz electron pocket's predominant interaction with the yz parts of the hole pockets is not an artifact of the approximation. We perform the mean-field calculation in a rotated basis with orbitals |a〉 =cosα | xz 〉 +sinα | yz 〉 and |b〉 =-sinα | xz 〉 +cosα | yz 〉 (Ref.) and find that (i) the energy is minimal for the original α=0 and that (ii) myz > mxz persists for α≠0
- Since our mean-field approach breaks the orbital symmetry by neglecting the "pair-hopping" and spin-flip terms of the onsite interaction, we have to check that the y z electron pocket's predominant interaction with the y z parts of the hole pockets is not an artifact of the approximation. We perform the mean-field calculation in a rotated basis with orbitals | a 〉 = cos α | x z 〉 + sin α | y z 〉 and | b 〉 = - sin α | x z 〉 + cos α | y z 〉 (Ref.) and find that (i) the energy is minimal for the original α = 0 and that (ii) m y z > m x z persists for α≠0.

29
- 77955437338
- For the intermediate- U regime with small ordered moment, the (π,0 ) phase has actually slightly higher energy than a (π,π ) -AF phase with large ordered moment but since the five-band model is widely used by several authors, we are nevertheless going to discuss its properties under the assumption of (π,0 ) order
- For the intermediate- U regime with small ordered moment, the (π, 0) phase has actually slightly higher energy than a (π, π) -AF phase with large ordered moment but since the five-band model is widely used by several authors, we are nevertheless going to discuss its properties under the assumption of (π, 0) order.

30
- 65149100538
- 10.1103/PhysRevB.79.134502
- A. Moreo, M. Daghofer, J. A. Riera, and E. Dagotto, Phys. Rev. B 79, 134502 (2009). 10.1103/PhysRevB.79.134502
- (2009) Phys. Rev. B , vol.79 , pp. 134502
- Moreo, A.¹ Daghofer, M.² Riera, J.A.³ Dagotto, E.⁴

31
- 69149096899
- 10.1143/JPSJ.78.083704
- K. Kubo and P. Thalmeier, J. Phys. Soc. Jpn. 78, 083704 (2009). 10.1143/JPSJ.78.083704
- (2009) J. Phys. Soc. Jpn. , vol.78 , pp. 083704
- Kubo, K.¹ Thalmeier, P.²

32
- 0000082395
- 10.1103/PhysRevLett.74.4281
- S. Haas, A. Moreo, and E. Dagotto, Phys. Rev. Lett. 74, 4281 (1995). 10.1103/PhysRevLett.74.4281
- (1995) Phys. Rev. Lett. , vol.74 , pp. 4281
- Haas, S.¹ Moreo, A.² Dagotto, E.³

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