Canonical dynamics: Equilibrium phase-space distributionsby: William G Hoover
Physical Review A, Vol. 31, No. 3. (March 1985), 1695.
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Notes for this articlenose-hoover thermostat intro
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AbstractNosé has modified Newtonian dynamics so as to reproduce both the canonical and the isothermal-isobaric probability densities in the phase space of an N -body system. He did this by scaling time (with s) and distance (with V 1/ D in D dimensions) through Lagrangian equations of motion. The dynamical equations describe the evolution of these two scaling variables and their two conjugate momenta p s and p v . Here we develop a slightly different set of equations; free of time scaling. We find the dynamical steady-state probability density in an extended phase space with variables x ; p x ; V ; ε̇ ; and ζ ; where the x are reduced distances and the two variables ε̇ and ζ act as thermodynamic friction coefficients. We find that these friction coefficients have Gaussian distributions. From the distributions the extent of small-system non-Newtonian behavior can be estimated. We illustrate the dynamical equations by considering their application to the simplest possible case; a one-dimensional classical harmonic oscillator.
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