A world-line Monte Carlo approach is proposed to calculate the elementary excitations of quantum systems. The lowest energies as a function of momentum are successfully extracted from an imaginary-time correlation function evaluated at a sufficiently low temperature. The method is applied to the antiferromagnetic Heisenberg chains of
S=21,1,23, and
2 with length up to 64. The spectra for
S=21 and 1 coincide well with the result by des Cloizeaux and Pearson and with the result by Takahashi, respectively. The spectra for
S=23 and 2 turn out to be massless and massive, respectively. The
S=2 Haldane gap is estimated to be $0.049\ifmmode\pm\else\textpm\fi{}0.018$.
A world-line quantum Monte Carlo method is employed to study the elementary excitations of S=1 antiferromagnetic Heisenberg chains with bond alternation described by the Hamiltonian, scrH=J
tsumi [1-(-1
)i\ensuremath{\delta}]
Si\ensuremath{\cdot}
Si+1. Imaginary-time correlation functions of this system at low-enough temperatures exhibit almost single-exponential decay and thus the lowest excitation spectrum can be successfully extracted from them. As \ensuremath{\delta} increases from 0 to 1, the system encounters a continuous phase transition at \ensuremath{\delta}\ensuremath{\simeq}0.25, where the energy(E)-momentum(q) relation is fitted well to the form E(q)=(
v2 sin2q+${\mathrm{\ensuremath{\Delta}}}^{2}$
)1/2 with the effective light velocity v=2.46\ifmmode\pm\else\textpm\fi{}0.08 and the energy gap \ensuremath{\Delta} which vanishes in the long chain limit. The central charge c at the massless critical point is estimated to be 1.02\ifmmode\pm\else\textpm\fi{}0.09, which suggests the universality class of the Gaussian model.
The elementary excitations of the one-dimensional spin-S Heisenberg antiferromagnet near saturation are explained, with special attention to the soft mode, in terms of a gas of interacting magnons. Recent numerical studies of the antiferromagnet in a magnetic field uncovered the presence of the soft mode at a magnetization-dependent wave number for large magnetizations. We show that very near saturation and for large spins the antiferromagnet can be written in terms of a gas of magnons interacting via repulsive \ensuremath{\delta}-function potentials, a system with a known Bethe-ansatz solution. The soft mode can then be explained as a Kohn-anomaly-type excitation above a quasi-Fermi-sea. Other elementary excitations form a particle-hole-type double continuum. The soft mode's apparent physical observability is indicated by a shoulder at the appropriate wave number in the integrated longitudinal intensity.