Approach to Equilibrium of Statistical Systems: Classical Particles and Quantum Fields Off-Equilibrium

R. F. Álvarez-Estrada
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Abstract

Non-equilibrium evolution at absolute temperature T and approach to equilibrium of statistical systems in long-time (t) approximations, using both hierarchies and functional integrals, are reviewed. A classical non-relativistic particle in one spatial dimension, subject to a potential and a heat bath (hb), is described by the non-equilibrium reversible Liouville distribution (W) and equation, with a suitable initial condition. The Boltzmann equilibrium distribution Weq generates orthogonal (Hermite) polynomials Hn in momenta. Suitable moments Wn of W (using the Hn’s) yield a non-equilibrium three-term hierarchy (different from the standard Bogoliubov–Born–Green–Kirkwood–Yvon one), solved through operator continued fractions. After a long-t approximation, the Wn’s yield irreversibly approach to equilibrium. The approach is extended (without hb) to: (i) a non-equilibrium system of N classical non-relativistic particles interacting through repulsive short range potentials and (ii) a classical ϕ4 field theory (without hb). The extension to one non-relativistic quantum particle (with hb) employs the non-equilibrium Wigner function (WQ): difficulties related to non-positivity of WQ are bypassed so as to formulate approximately approach to equilibrium. A non-equilibrium quantum anharmonic oscillator is analyzed differently, through functional integral methods. The latter allows an extension to relativistic quantum ϕ4 field theory (a meson gas off-equilibrium, without hb), facing ultraviolet divergences and renormalization. Genuine simplifications of quantum ϕ4 theory at high T and large distances and long t occur; then, through a new argument for the field-theoretic case, the theory can be approximated by a classical ϕ4 one, yielding an approach to equilibrium.
统计系统的平衡方法:经典粒子和非平衡量子场
在绝对温度T下的非平衡演化和统计系统在长时间(T)近似下的平衡方法,使用层次和泛函积分进行了回顾。在一个合适的初始条件下,用非平衡可逆Liouville分布(W)和方程来描述一维空间中的经典非相对论性粒子,该粒子具有势和热浴(hb)。玻尔兹曼平衡分布Weq在动量上产生正交(Hermite)多项式Hn。合适的矩W(使用Hn)产生一个非平衡的三项层次结构(不同于标准的Bogoliubov-Born-Green-Kirkwood-Yvon),通过算子连分数求解。经过长t近似后,w 's不可逆地趋于平衡。该方法(没有hb)扩展到:(i) N个经典非相对论性粒子通过排斥性短程势相互作用的非平衡系统和(ii)经典的ϕ4场论(没有hb)。对一个非相对论量子粒子(带hb)的扩展采用了非平衡维格纳函数(WQ):绕过了与WQ非正性有关的困难,从而形成了近似的平衡方法。利用泛函积分方法对非平衡态量子非谐振子进行了不同的分析。后者允许扩展到相对论量子场理论(介子气体失去平衡,没有hb),面对紫外线发散和重整化。在高T、大距离和长T下,量子ϕ4理论得到了真正的简化;然后,通过对场论情况的一个新的论证,该理论可以用经典的ϕ4近似,从而得到一种接近平衡的方法。
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