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Equilibrium free energies from fast-switching trajectories with large time steps

机译:具有大时间步长的快速切换轨迹的平衡自由能

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Jarzynski's [Phys. Rev. Lett. 78, 2690 (1997)] identity for the free-energy difference between two equilibrium states can be viewed as a special case of a more general procedure based on phase-space mappings. Solving a system's equation of motion by approximate means generates a mapping that is perfectly valid for this purpose, regardless of how closely the solution mimics true time evolution. We exploit this fact, using crudely dynamical trajectories to compute free-energy differences that are in principle exact. Numerical simulations show that Newton's equation can be discretized to low order over very large time steps (limited only by the computer's ability to represent resulting values of dynamical variables) without sacrificing thermodynamic accuracy. For computing the reversible work required to move a particle through a dense liquid, these calculations are more efficient than conventional fast-switching simulations by more than an order of magnitude. We also explore consequences of the phase-space mapping perspective for systems at equilibrium, deriving an exact expression for the statistics of energy fluctuations in simulated conservative systems. (c) 2006 American Institute of Physics.
机译:Jarzynski的[Phys。牧师[J.Am.Chem.Soc。,78,2690(1997)]关于两个平衡状态之间的自由能差的同一性可以被视为基于相空间映射的更通用程序的特例。用近似方法求解系统的运动方程会生成一个映射,该映射对于此目的是完全有效的,而与解决方案模拟真实时间演化的紧密程度无关。我们利用这一事实,使用粗略的动力学轨迹来计算原则上精确的自由能差异。数值模拟表明,牛顿方程可以在很大的时间步长上离散为低阶(仅受计算机表示动态变量结果值的能力限制)而不会牺牲热力学精度。为了计算使粒子移动通过稠密液体所需的可逆功,这些计算比常规的快速切换模拟效率高出一个数量级。我们还探讨了相空间映射透视图对处于平衡状态的系统的影响,从而得出了模拟保守系统中能量波动统计的精确表达式。 (c)2006年美国物理研究所。

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