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Volumn 83, Issue 17, 2011, Pages

Critical spin dynamics of the S=12 spin chain compound CuSe 2O5

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EID: 79961068868     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.83.174413     Document Type: Article
Times cited : (20)

References (36)
  • 1
    • 0037307241 scopus 로고    scopus 로고
    • Magnetic light scattering in low-dimensional quantum spin systems
    • DOI 10.1016/S0370-1573(02)00321-6, PII S0370157302003216
    • P. Lemmens, G. Güntherodt, and C. Gros, Phys. Rep. PRPLCM 0370-1573 10.1016/S0370-1573(02)00321-6 375, 1 (2003). (Pubitemid 36140471)
    • (2003) Physics Report , vol.375 , Issue.1 , pp. 1-103
    • Lemmens, P.1    Guntherodt, G.2    Gros, C.3
  • 2
    • 33846900525 scopus 로고
    • EPJAFV 1434-6001 10.1007/BF01341708
    • H. Bethe, Z. Phys. EPJAFV 1434-6001 10.1007/BF01341708 71, 205 (1931).
    • (1931) Z. Phys. , vol.71 , pp. 205
    • Bethe, H.1
  • 3
    • 1542792942 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.70.3651
    • M. Hase, I. Terasaki, and K. Uchinokura, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.70.3651 70, 3651 (1993).
    • (1993) Phys. Rev. Lett. , vol.70 , pp. 3651
    • Hase, M.1    Terasaki, I.2    Uchinokura, K.3
  • 7
    • 0000980809 scopus 로고
    • PYLAAG 0375-9601 10.1016/0375-9601(92)90823-5
    • K. Okamoto and K. Nomura, Phys. Lett. A PYLAAG 0375-9601 10.1016/0375-9601(92)90823-5 169, 433 (1992).
    • (1992) Phys. Lett. A , vol.169 , pp. 433
    • Okamoto, K.1    Nomura, K.2
  • 9
    • 33646661501 scopus 로고
    • JUPSAU 0031-9015 10.1143/JPSJ.58.2902
    • T. Tonegawa and I. Harada, J. Phys. Soc. Jpn. JUPSAU 0031-9015 10.1143/JPSJ.58.2902 58, 2902 (1989).
    • (1989) J. Phys. Soc. Jpn. , vol.58 , pp. 2902
    • Tonegawa, T.1    Harada, I.2
  • 10
    • 6144284465 scopus 로고    scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.77.2790
    • H. J. Schulz, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.77. 2790 77, 2790 (1996).
    • (1996) Phys. Rev. Lett. , vol.77 , pp. 2790
    • Schulz, H.J.1
  • 11
    • 0000231970 scopus 로고    scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.56.11001
    • F. H. L. Essler, A. M. Tsvelik, and G. Delfino, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.56.11001 56, 11001 (1997).
    • (1997) Phys. Rev. B , vol.56 , pp. 11001
    • Essler, F.H.L.1    Tsvelik, A.M.2    Delfino, G.3
  • 13
    • 48749123425 scopus 로고    scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.78.014429
    • A. A. Zvyagin and S.-L. Drechsler, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.78.014429 78, 014429 (2008).
    • (2008) Phys. Rev. B , vol.78 , pp. 014429
    • Zvyagin, A.A.1    Drechsler, S.-L.2
  • 14
    • 0001155754 scopus 로고    scopus 로고
    • Irkhin and, PRBMDO 1098-0121 10.1103/PhysRevB.61.6757
    • V. Yu. Irkhin and A. A. Katanin, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.61.6757 61, 6757 (2000).
    • (2000) Phys. Rev. B , vol.61 , pp. 6757
    • Yu, V.1    Katanin, A.A.2
  • 15
    • 0001747790 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.13.169
    • G. F. Reiter, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.13.169 13, 169 (1976).
    • (1976) Phys. Rev. B , vol.13 , pp. 169
    • Reiter, G.F.1
  • 16
    • 4243228448 scopus 로고
    • PRLTAO 0031-9007 10.1103/PhysRevLett.41.1605
    • J. W. Halley, Phys. Rev. Lett. PRLTAO 0031-9007 10.1103/PhysRevLett.41. 1605 41, 1605 (1978).
    • (1978) Phys. Rev. Lett. , vol.41 , pp. 1605
    • Halley, J.W.1
  • 17
    • 36049054308 scopus 로고
    • PHRVAO 0031-899X 10.1103/PhysRev.188.898
    • B. I. Halperin and P. C. Hohenberg, Phys. Rev. PHRVAO 0031-899X 10.1103/PhysRev.188.898 188, 898 (1969).
    • (1969) Phys. Rev. , vol.188 , pp. 898
    • Halperin, B.I.1    Hohenberg, P.C.2
  • 18
    • 0012850427 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.9.2244
    • W. J. Brya and P. M. Richards, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.9.2244 9, 2244 (1974).
    • (1974) Phys. Rev. B , vol.9 , pp. 2244
    • Brya, W.J.1    Richards, P.M.2
  • 19
    • 0012803151 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.9.3044
    • P. M. Richards and W. J. Brya, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.9.3044 9, 3044 (1974).
    • (1974) Phys. Rev. B , vol.9 , pp. 3044
    • Richards, P.M.1    Brya, W.J.2
  • 27
    • 34249890027 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.28.1928
    • M. Balkanski, R. F. Wallis, and E. Haro, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.28.1928 28, 1928 (1983).
    • (1983) Phys. Rev. B , vol.28 , pp. 1928
    • Balkanski, M.1    Wallis, R.F.2    Haro, E.3
  • 31
    • 0000983206 scopus 로고
    • PRBMDO 1098-0121 10.1103/PhysRevB.49.1048
    • I. Yamada and H. Onda, Phys. Rev. B PRBMDO 1098-0121 10.1103/PhysRevB.49. 1048 49, 1048 (1994).
    • (1994) Phys. Rev. B , vol.49 , pp. 1048
    • Yamada, I.1    Onda, H.2
  • 32
    • 79961038528 scopus 로고    scopus 로고
    • If quasielastic scattering contains two contributions from fluctuations of the spin energy density and a parallel component of the sublattice magnetization, it is described by a sum of two Lorentzian profiles. If diffusive fluctuations are present, a Gaussian profile should be added.
    • If quasielastic scattering contains two contributions from fluctuations of the spin energy density and a parallel component of the sublattice magnetization, it is described by a sum of two Lorentzian profiles. If diffusive fluctuations are present, a Gaussian profile should be added.
  • 33
    • 36049060679 scopus 로고
    • PHRVAO 0031-899X 10.1103/PhysRev.150.291
    • K. Kawasaki, Phys. Rev. PHRVAO 0031-899X 10.1103/PhysRev.150.291 150, 291 (1966).
    • (1966) Phys. Rev. , vol.150 , pp. 291
    • Kawasaki, K.1
  • 34
    • 0040841088 scopus 로고
    • PPSOAU 0370-1328 10.1088/0370-1328/90/3/324
    • K. Kawasaki and M. Tanaka, Proc. Phys. Soc. London PPSOAU 0370-1328 10.1088/0370-1328/90/3/324 90, 791 (1967).
    • (1967) Proc. Phys. Soc. London , vol.90 , pp. 791
    • Kawasaki, K.1    Tanaka, M.2
  • 36
    • 79961090261 scopus 로고    scopus 로고
    • N)μ. We found for both data sets μ=0.28. This value is close to what is expected for a 3D S=1/2 Heisenberg model.
    • N) μ. We found for both data sets μ = 0. 28. This value is close to what is expected for a 3D S = 1 / 2 Heisenberg model.


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