메뉴 건너뛰기




Volumn 83, Issue 17, 2011, Pages

Charge stripes in the two-orbital Hubbard model for iron pnictides

Author keywords

[No Author keywords available]

Indexed keywords


EID: 79961121917     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.83.174513     Document Type: Article
Times cited : (16)

References (33)
  • 1
    • 77957966305 scopus 로고    scopus 로고
    • ADPHAH 0001-8732 10.1080/00018732.2010.513480
    • For a recent review, see D. C. Johnston, Adv. Phys. ADPHAH 0001-8732 10.1080/00018732.2010.513480 59, 803 (2010), and references therein.
    • (2010) Adv. Phys. , vol.59 , pp. 803
    • Johnston, D.C.1
  • 3
    • 49749091616 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.101.076401
    • Q. Si and E. Abrahams, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.101.076401 101, 076401 (2008);
    • (2008) Phys. Rev. Lett. , vol.101 , pp. 076401
    • Si, Q.1    Abrahams, E.2
  • 4
    • 57749089579 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.101.206404
    • K. Seo, B. A. Bernevig, and J. Hu, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.101.206404 101, 206404 (2008);
    • (2008) Phys. Rev. Lett. , vol.101 , pp. 206404
    • Seo, K.1    Bernevig, B.A.2    Hu, J.3
  • 8
    • 45249110399 scopus 로고    scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.77.220503
    • S. Raghu, Xiao-Liang Qi, Chao-Xing Liu, D. J. Scalapino, and Shou-Cheng Zhang, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.77.220503 77, 220503 (2008).
    • (2008) Phys. Rev. B , vol.77 , pp. 220503
    • Raghu, S.1    Qi, X.2    Liu, C.3    Scalapino, D.J.4    Zhang, S.5
  • 18
    • 77649206048 scopus 로고    scopus 로고
    • As nuclear quadrupole results also indicate the presence of two charge environments in some "1111" pnictides, see 0031-9007 10.1103/PhysRevLett.104.097001
    • As nuclear quadrupole results also indicate the presence of two charge environments in some "1111" pnictides, see G. Lang, H.-J. Grafe, D. Paar, F. Hammerath, K. Manthey, G. Behr, J. Werner, and B. Büchner, Phys. Rev. Lett. 0031-9007 10.1103/PhysRevLett.104.097001 104, 097001 (2010).
    • (2010) Phys. Rev. Lett. , vol.104 , pp. 097001
    • Lang, G.1    Grafe, H.-J.2    Paar, D.3    Hammerath, F.4    Manthey, K.5    Behr, G.6    Werner, J.7    Büchner, B.8
  • 19
    • 0000697334 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.40.7391
    • J. Zaanen and O. Gunnarsson, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.40.7391 40, 7391 (1989);
    • (1989) Phys. Rev. B , vol.40 , pp. 7391
    • Zaanen, J.1    Gunnarsson, O.2
  • 20
    • 0001662278 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.39.9749
    • D. Poilblanc and T. M. Rice, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.39.9749 39, 9749 (1989);
    • (1989) Phys. Rev. B , vol.39 , pp. 9749
    • Poilblanc, D.1    Rice, T.M.2
  • 21
    • 0024641477 scopus 로고
    • 0921-4534 10.1016/0921-4534(89)90316-X
    • K. Machida, Physica C 0921-4534 10.1016/0921-4534(89)90316-X 158, 192 (1989);
    • (1989) Physica C , vol.158 , pp. 192
    • MacHida, K.1
  • 24
    • 47049098637 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.101.026403
    • L. Boeri, O. V. Dolgov, and A. A. Golubov, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.101.026403 101, 026403 (2008).
    • (2008) Phys. Rev. Lett. , vol.101 , pp. 026403
    • Boeri, L.1    Dolgov, O.V.2    Golubov, A.A.3
  • 26
    • 0001374756 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.28.327
    • A. M. Ole, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.28.327 28, 327 (1983).
    • (1983) Phys. Rev. B , vol.28 , pp. 327
    • Ole, A.M.1
  • 27
    • 79961112869 scopus 로고    scopus 로고
    • See supplemental material at [http://link.aps.org/supplemental/10.1103/ PhysRevB.83.174513] for the full HF Hamiltonian.
  • 28
    • 0000738606 scopus 로고
    • The method used is described in, PRBMDO 1098-0121 10.1103/PhysRevB.38. 12807
    • The method used is described in D. D. Johnson, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.38.12807 38, 12807 (1988), with a linear mixing parameter α = 0. 5.
    • (1988) Phys. Rev. B , vol.38 , pp. 12807
    • Johnson, D.D.1
  • 29
    • 55749101372 scopus 로고    scopus 로고
    • Densities n very close to 2.0 will not be explored due to the competition of other states [, PRLTAO 0031-9007 10.1103/PhysRevLett.101.186402
    • Densities n very close to 2.0 will not be explored due to the competition of other states [J. Lorenzana, G. Seibold, C. Ortix, and M. Grilli, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.101.186402 101, 186402 (2008)] that are not the focus of our effort.
    • (2008) Phys. Rev. Lett. , vol.101 , pp. 186402
    • Lorenzana, J.1    Seibold, G.2    Ortix, C.3    Grilli, M.4
  • 30
    • 59449110913 scopus 로고    scopus 로고
    • PRLTAO 1745-2473 10.1038/nphys1160
    • I. I. Mazin and M. D. Johannes, Nat. Phys. PRLTAO 1745-2473 10.1038/nphys1160 5, 141 (2008).
    • (2008) Nat. Phys. , vol.5 , pp. 141
    • Mazin, I.I.1    Johannes, M.D.2
  • 32
    • 77956307791 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.105.107004
    • Wei-Guo Yin, Chi-Cheng Lee, and Wei Ku, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.105.107004 105, 107004 (2010).
    • (2010) Phys. Rev. Lett. , vol.105 , pp. 107004
    • Yin, W.1    Lee, C.2    Ku, W.3
  • 33
    • 0037720481 scopus 로고    scopus 로고
    • PRPLCM 0370-1573 10.1016/S0370-1573(00)00121-6
    • E. Dagotto, T. Hotta, and A. Moreo, Phys. Rep. PRPLCM 0370-1573 10.1016/S0370-1573(00)00121-6 344, 1 (2001).
    • (2001) Phys. Rep. , vol.344 , pp. 1
    • Dagotto, E.1    Hotta, T.2    Moreo, A.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.