We have investigated the magnetic susceptibility of three quasiclassical one-dimensional magnetic systems, CsMnBr₃, (CH₃{)}₄NMnCl₃ (TMMC), and CH₃{NH}₃MnCl₃{·}2H₂O (MMC), in their paramagnetic regimes. We find that a previous analysis in terms of a classical Heisenberg Hamiltonian does not provide an adequate description of the data at low temperatures where short-range correlations are high. We show that approximate quantum-mechanical corrections to this exact treatment do not account for the discrepancies systematically. A classical treatment which includes exchange interactions biquadratic in the spins is applied to this problem, resulting in a marked improvement of the description of experiments by theory at all temperatures. We include weak dipolar terms in the Hamiltonian, in addition to both bilinear and biquadratic exchange terms, for the case of CsMnBr₃ by means of a Monte Carlo simulation. To within the quoted accuracy, the simulation describes the susceptibility completely for the temperature range considered. Our results show that the strength of the biquadratic exchange interactions, relative to the strength of the bilinear interactions, is strongest in MMC and weakest in TMMC, but that the absolute magnitude is greatest for CsMnBr₃. Quantitatively, we find that our calculations produce a biquadratic exchange strength for CsMnBr₃ which is in agreement with neutron spectroscopic measurements of transition energies in Mn²⁺ linear triads.
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Gaulin et al. (1986) studied this question.
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