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双缝实验中波函数退相和退相干的微观模型。

A microscopic model of wave-function dephasing and decoherence in the double-slit experiment.

作者信息

Ramakrishna Satish

机构信息

Department of Physics and Astronomy, Rutgers, The State University of New Jersey, 136 Frelinghuysen Road, Piscataway, NJ, 08854-8019, USA.

出版信息

Sci Rep. 2021 Oct 25;11(1):20986. doi: 10.1038/s41598-021-99995-2.

Abstract

The act of measurement on a quantum state is supposed to "dephase" (dephasing refers to the phenomenon that the states lose phase coherence; then the phases get randomized in interaction with a bath of other oscillators, which is referred to as "decoherence"), then "decohere" and "collapse" (or more precisely "register" and "reduce") the state into one of several eigenstates of the operator corresponding to the observable being measured. This measurement process is sometimes described as outside standard quantum-mechanical evolution and not calculable from Schrödinger's equation. Progress has, however, been made in studying this problem with two main calculation tools-one uses a time-independent Hamiltonian, while a rather more general approach proving that decoherence occurs under some generic conditions. The two general approaches to the study of wave-function collapse are as follows. The first approach, called the "consistent" or "decoherent"' histories approach, studies microscopic histories that diverge probabilistically and explains collapse as an event in our particular history. The other, referred to as the "environmental decoherence" approach studies the effect of the environment upon the quantum system, to explain wave-function decoherence which is produced by irreversible effects of various sorts. However, as we know, wave-function collapse is not related to thermal connection with the environment, rather, it is inherent to how measurements are performed by macroscopic apparata. In the "environmental decoherence" approach, one studies decoherence using a Markovian-approximated Master equation to study the time-evolution of the reduced density matrix (post dephasing) and obtains the long-time dependence of the off-diagonal elements of this matrix. The calculation in this paper studies the evolution of a quantum system starting with "dephasing" followed by the effects of the environment with some differences from prior analyses. We start from the Schrödinger equation for the state of the system, with a time-dependent Hamiltonian that reflects the actual microscopic interactions that are occurring. Then we systematically solve (exactly) for the time-evolved state, without invoking a Markovian approximation when writing out the effective time-evolution equation, i.e., keeping the evolution unitary until the end. This approach is useful, and it shows that the system wave-function will explicitly "un-collapse" if the measurement apparatus is sufficiently small. However, in the limit of a macroscopic system, this "dephasing" quickly leads to "decoherence"-collapse is a temporary state that will simply take extremely long (of the order of multiple universe lifetimes) to reverse. This has been attempted previously and our calculation is particularly simple and calculable. We make some connections to the work by Linden et al. while doing so. The calculation in this paper has interesting implications for the interpretation of the Wigner's friend experiment, as well as the Mott experiment, which is explored in "Connection to some general theoretical results" and "Recurrence times" (especially the enumerated points in "Recurrence times"). The upshot is that as long as Wigner's friend is macroscopically large (or uses a macroscopically large measuring instrument), no one needs to worry that Wigner would see something different from his friend. Indeed, Wigner's friend does not even need to be conscious during the measurement that she conducts. It also allows one to reasonably interpret some of the more recent thought experiments proposed. In particular, as a result of the mathematical analysis, the short-time behavior of a collapsing system, at least the one considered in this paper, is not exponential. Instead, it is the usual Fermi-golden rule result. The long-term behavior is, of course, still exponential. This is a second novel feature of the paper-we connect the short-term Fermi-golden rule (quadratic-in-time behavior) transition probability to the exponential long-time behavior of a collapsing wave-function in one continuous mathematical formulation.

摘要

对量子态进行测量的行为被认为会导致“去相位”(去相位是指态失去相位相干性的现象;随后相位在与其他振荡器组成的“热库”相互作用中随机化,这被称为“退相干”),然后使态“退相干”并“坍缩”(或更准确地说是“记录”和“约化”)为与所测量可观测量对应的算符的几个本征态之一。这种测量过程有时被描述为超出标准量子力学演化的范畴,无法从薛定谔方程计算得出。然而,在使用两种主要计算工具研究这个问题方面已经取得了进展——一种使用与时间无关的哈密顿量,而另一种更通用的方法证明了在某些一般条件下会发生退相干。研究波函数坍缩的两种一般方法如下。第一种方法,称为“一致”或“退相干历史”方法,研究概率性发散的微观历史,并将坍缩解释为我们特定历史中的一个事件。另一种方法,称为“环境退相干”方法,研究环境对量子系统的影响,以解释由各种不可逆效应产生的波函数退相干。然而,正如我们所知,波函数坍缩与与环境的热联系无关,相反,它是宏观仪器进行测量方式所固有的。在“环境退相干”方法中,人们使用马尔可夫近似主方程来研究约化密度矩阵(去相位之后)的时间演化,并得到该矩阵非对角元素的长时间依赖性。本文中的计算研究了一个量子系统的演化,从“去相位”开始,接着是环境的影响,与之前的分析有一些不同。我们从系统状态的薛定谔方程出发,其哈密顿量与时间有关,反映了实际发生的微观相互作用。然后我们系统地(精确地)求解时间演化后的状态,在写出有效时间演化方程时不引入马尔可夫近似,即保持演化的幺正性直到最后。这种方法很有用,并且表明如果测量仪器足够小,系统波函数将明确地“恢复坍缩前状态”。然而,在宏观系统的极限情况下,这种“去相位”会迅速导致“退相干”——坍缩是一种暂时状态,只是要花费极长的时间(多个宇宙寿命的量级)才能逆转。这在之前已经有人尝试过,并且我们的计算特别简单且可计算。在这样做的过程中,我们与林登等人的工作建立了一些联系。本文中的计算对维格纳朋友实验以及莫特实验的解释有有趣的启示,这在“与一些一般理论结果的联系”和“回归时间”(特别是“回归时间”中列举的要点)中进行了探讨。结果是,只要维格纳的朋友在宏观上足够大(或者使用宏观上足够大的测量仪器),就没有人需要担心维格纳会看到与他的朋友不同的东西。实际上,维格纳的朋友在她进行测量的过程中甚至不需要有意识。它还使人们能够合理地解释一些最近提出的思想实验。特别是,由于数学分析的结果,坍缩系统的短时间行为,至少是本文所考虑的系统,不是指数形式的。相反,它是通常的费米黄金规则结果。当然,长时间行为仍然是指数形式的。这是本文的第二个新颖之处——我们在一个连续的数学公式中将短时间费米黄金规则(时间二次行为)跃迁概率与坍缩波函数的指数长时间行为联系起来。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/b902/8545942/321bbb68e216/41598_2021_99995_Fig1_HTML.jpg

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