Microcanonical solution of the mean-field model: comparison with time averages at finite size
arXiv:cond-mat/0509030 · doi:10.1016/j.physa.2006.01.066
Abstract
We solve the mean-field model in an external magnetic field in the microcanonical ensemble using two different methods. The first one is based on Rugh's microcanonical formalism and leads to express macroscopic observables, such as temperature, specific heat, magnetization and susceptibility, as time averages of convenient functions of the phase-space. The approach is applicable for any finite number of particles . The second method uses large deviation techniques and allows us to derive explicit expressions for microcanonical entropy and for macroscopic observables in the limit. Assuming ergodicity, we evaluate time averages in molecular dynamics simulations and, using Rugh's approach, we determine the value of macroscopic observables at finite . These averages are affected by a slow time evolution, often observed in systems with long-range interactions. We then show how the finite time averages of macroscopic observables converge to their corresponding values as is increased. As expected, finite size effects scale as .
arXiv comment18 pages, 1 figure
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Cited by in corpus (7)
- The large deviation approach to statistical mechanics
- Statistical mechanics and dynamics of solvable models with long-range interactions
- Phase transitions and configuration space topology
- Negative magnetic susceptibility and nonequivalent ensembles for the mean-field spin model
- On the thermodynamics of classical micro-canonical systems
- Stability of inhomogeneous states in mean-field models with a local potential
- Quantum fluctuations inhibit symmetry breaking in the HMF model