2000
DOI: 10.1103/physreve.61.3579
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Dynamical temperature for spin systems

Abstract: A transcription of Rugh's geometrical approach to temperature is given for classical Heisenberg spin systems. For the simple case of a paramagnet with small and large numbers of spins we verify the approach. A numerical check for long spin chains using spin dynamics shows its practicality.

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Cited by 37 publications
(27 citation statements)
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“…The initial state for the time integration was generated from the procedure described in Sec. II C. The spin temperature was measured using the formula developed by Nurdin et al [53].…”
Section: Simulation Detailsmentioning
confidence: 99%
“…The initial state for the time integration was generated from the procedure described in Sec. II C. The spin temperature was measured using the formula developed by Nurdin et al [53].…”
Section: Simulation Detailsmentioning
confidence: 99%
“…Instead of three components for the classical Heisenberg system in our preliminary paper [3], here we want to study the simpler XY -spin system where only two components S = S 1 , S 2 have to be taken into account, that is the spin vector is confined to a circle with radius S. No dynamical equation can be written down similar to ∂ S ∂t = S × H for the three dimensional vector S in a magnetic field H. The energy − H · S = −H S cos ϕ is the same for the two directions ±ϕ the vector S can point. Contrary to the three dimensional case, there is no continuous path between these equal energy states at ±ϕ.…”
Section: A General Approachmentioning
confidence: 99%
“…Although the energy is conserved one can determine the temperature for a system consisting of kinetic and potential energy the temperature by the average kinetic energy. With the recent advance in the understanding of the micro-canonical temperature initiated by Rugh [1][2][3], one can "measure" the temperature and also the specific heat along the trajectory of spin systems where such a decomposition of the energy does not exist. In the case of XY-spins one could also add the sum over the angular velocities but a dynamical check of statistical mechanics by a common molecular dynamics simulation is not an easy numerical task [4].…”
Section: Introductionmentioning
confidence: 99%
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“…Considering the square of this function one may in addition consider fluctuations of the inverse temperature. In case the ergodic hypothesis holds such averages may then be written as time averages using the dynamics of the classical Hamilton function (see, e.g., [67,68,5,60]). An important feature of a microcanonical ensemble is that the temperature may decrease with energy giving rise to a negative heat capacity.…”
Section: Introductionmentioning
confidence: 99%