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A canonical averaging in the second-order quantized Hamilton dynamics

机译:二阶量化汉密尔顿动力学的典范平均

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Quantized Hamilton dynamics (QHD) is a simple and elegant extension of classical Hamilton dynamics that accurately includes zero-point energy, tunneling, dephasing, and other quantum effects. Formulated as a hierarchy of approximations to exact quantum dynamics in the Heisenberg formulation, QHD has been used to study evolution of observables subject to a single initial condition. In present, we develop a practical solution for generating canonical ensembles in the second-order QHD for position and momentum operators, which can be mapped onto classical phase space in doubled dimensionality and which in certain limits is equivalent to thawed Gaussian. We define a thermal distribution in the space of the QHD-2 variables and show that the standard beta=1/kT relationship becomes beta(')=2/kT in the high temperature limit due to an overcounting of states in the extended phase space, and a more complicated function at low temperatures. The QHD thermal distribution is used to compute total energy, kinetic energy, heat capacity, and other canonical averages for a series of quartic potentials, showing good agreement with the quantum results. (C) 2004 American Institute of Physics.
机译:量子汉密尔顿动力学(QHD)是经典汉密尔顿动力学的简单而优雅的扩展,它精确地包括零点能量,隧穿,相移和其他量子效应。 QHD被公式化为海森堡公式中精确量子动力学的近似层次,已被用于研究在单个初始条件下可观测物的演化。目前,我们为位置和动量算子开发了用于生成二阶QHD典范合奏的实用解决方案,可以将其以二维方式映射到经典相空间,并且在某些限制下等效于解冻的高斯。我们定义了QHD-2变量空间中的热分布,并表明由于扩展相空间中状态的过度计数,在高温极限下,标准beta = 1 / kT关系变为beta(')= 2 / kT ,并且在低温下功能更为复杂。 QHD热分布用于计算一系列四次势的总能量,动能,热容量和其他规范平均值,与量子结果显示出很好的一致性。 (C)2004年美国物理研究所。

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