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Volumn 11, Issue 17, 1997, Pages 2057-2074

Spin and charge density waves in the extended Hubbard model: A slave-boson approach

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EID: 0004024002     PISSN: 02179792     EISSN: None     Source Type: Journal    
DOI: 10.1142/S0217979297001064     Document Type: Article
Times cited : (8)

References (22)
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    • B. Fourcade and G. Spronken, Phys. Rev. B29, 5089 (1984); ibid. 5096 (1984).
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  • 8
    • 0000894335 scopus 로고
    • P. G. J. van Dongen, Phys. Rev. B29, 14016 (1994); Phys. Rev. Lett. 74, 182 (1995).
    • (1994) Phys. Rev. , vol.B29 , pp. 14016
    • Van Dongen, P.G.J.1
  • 9
    • 6144237781 scopus 로고
    • P. G. J. van Dongen, Phys. Rev. B29, 14016 (1994); Phys. Rev. Lett. 74, 182 (1995).
    • (1995) Phys. Rev. Lett. , vol.74 , pp. 182
  • 10
    • 0000459283 scopus 로고
    • S. E. Barnes, J. Phys. F6, 1375 (1976); P. Coleman, Phys. Rev. B29, 3035 (1984).
    • (1976) J. Phys. , vol.F6 , pp. 1375
    • Barnes, S.E.1
  • 11
    • 24444467134 scopus 로고
    • S. E. Barnes, J. Phys. F6, 1375 (1976); P. Coleman, Phys. Rev. B29, 3035 (1984).
    • (1984) Phys. Rev. , vol.B29 , pp. 3035
    • Coleman, P.1
  • 13
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    • H. Hasegawa, J. Phys. Condens. Mutt. 1, 9325 (1989); Phys. Rev. B41, 9168 (1990).
    • (1990) Phys. Rev. , vol.B41 , pp. 9168
  • 14
    • 0042319742 scopus 로고
    • For a similar approach in the case of the U ⇀ ∞ three-band Hubbard model see e.g. S. Caprara, C. Di Castro and M. Grilli, Phys. Rev. B51, 9286 (1995).
    • (1995) Phys. Rev. , vol.B51 , pp. 9286
    • Caprara, S.1    Di Castro, C.2    Grilli, M.3
  • 18
    • 85033135626 scopus 로고    scopus 로고
    • note
    • i,σ factors are possible, which give the correct matrix elements in the new Fock space, but give rise to different mean-field results. We made our choice according to Ref. 11 in order to have the correct U ⇁ 0 limiting behavior in our mean-field approximation.
  • 20
    • 85033136347 scopus 로고    scopus 로고
    • note
    • BR = 32t/π for d = 1), by equating to zero the coefficient of the logaritmically divergent part of the integral in the r.h.s of the second equation in (9), for m → 0.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.