1997
DOI: 10.1103/physrevb.56.645
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Quantum transfer-matrix approach toS=1antiferromagnetic chains at finite temperatures

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Cited by 20 publications
(14 citation statements)
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“…The best-fit parameters found for NENP, CsΝiCl3 , and YBANO are the following: J/kB = 48 K, D/kB = 7.8 K, gl = 2.25, g|| = 2.20; J/kB = 27 K, D/kB = 1.35 K, g = 2.23; J/kB = 275 K, D/kB = 60 K, g = 2.33, respectively. The simulations also imply some theoretical consequences as far as the boson and fermion approximations and strong anisotropy calculations are concerned [10].…”
Section: Resultsmentioning
confidence: 99%
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“…The best-fit parameters found for NENP, CsΝiCl3 , and YBANO are the following: J/kB = 48 K, D/kB = 7.8 K, gl = 2.25, g|| = 2.20; J/kB = 27 K, D/kB = 1.35 K, g = 2.23; J/kB = 275 K, D/kB = 60 K, g = 2.33, respectively. The simulations also imply some theoretical consequences as far as the boson and fermion approximations and strong anisotropy calculations are concerned [10].…”
Section: Resultsmentioning
confidence: 99%
“…Extensive large-scale simulations in the interval of parameters appropriate for NENP and other quasi-one-dimensional chains were also performed [10]. The best-fit parameters found for NENP, CsΝiCl3 , and YBANO are the following: J/kB = 48 K, D/kB = 7.8 K, gl = 2.25, g|| = 2.20; J/kB = 27 K, D/kB = 1.35 K, g = 2.23; J/kB = 275 K, D/kB = 60 K, g = 2.33, respectively.…”
Section: Resultsmentioning
confidence: 99%
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“…Analysis of our model (3) is based on the numerical Quantum Transfer Matrix method [20][21][22][23][24] , where the partition function of the quantum chain is mapped onto the partition function of the classical 2d system with multispin interactions and a finite width 2M 25,26 . For different values of M , called the Trotter number, the classical partition functions form a series of approximants Z M , where the leading errors are of the order of 1/M 2 .…”
Section: Model and Dmrg Methods For Canted Single-chain Magnetsmentioning
confidence: 99%
“…The QTM technique has been applied successfully to a number of the linear spin systems [5][6][7]. In order to perform numerical calculations for a macroscopic chain, we have first divided the Hamiltonian (1) into two parts H = HA + HR Then we used the Trotter expansion to obtain the m-th classical approximant Zm of the partition function Ζ of the classical system of 2m x N spins with the effective interactions grouped into eight-spin blocks Secondly, we introduced an effective classical spin σ = 3/2 to replace pairs of S = 1/2 spins distributed along each row r At the same step, we rewrote the local transfer matrix in the basis of σ.…”
Section: Qtm Techniquementioning
confidence: 99%