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薛定谔-牛顿半经典引力场景中的玻恩规则

Born rule in Schroedinger-Newton scenarios of semiclassical gravity

Tanguy Fontana, Axelle Coulon, Giovanni Manfredi

arXiv 2610.03501首次发表:更新:

发表机构

Université de Strasbourg, CNRS, Institut de Physique et Chimie des Matériaux de Strasbourg(斯特拉斯堡大学,法国国家科学研究中心,斯特拉斯堡材料物理与化学研究所)

机构由 AI 辅助整理,请以论文原文为准。

AI 中文总结

研究薛定谔-牛顿半经典引力模型中玻恩规则的动力学弛豫,发现波包有界或缓慢增长时弛豫发生,快速膨胀时偏离持续,数值模拟证实,为原始量子非平衡提供最小模型。

AI 中文摘要

我们研究了由薛定谔-牛顿方程描述的半经典引力模型中对玻恩规则的动力学弛豫。利用自引力波包的Gaussian变分解,结合Nelson的量子动力学随机表示,我们追踪了初始概率分布不同于$|\Psi|^2$的粒子系综的演化。当波包保持有界或随时间增长足够缓慢时,会发生对玻恩规则的弛豫(“量子平衡”);相反,对于薛定谔-牛顿方程的快速膨胀解,对玻恩规则的偏离可以无限期持续。数值模拟证实了这一分析图像。这些结果表明,半经典自引力既可以促进也可以抑制向玻恩规则的弛豫,为Underwood和Valentini [Phys. Rev. D 92, 063531 (2015)]提出的原始量子非平衡提议提供了一个最小模型。

英文摘要

We investigate dynamical relaxation to the Born rule in a semiclassical gravity model described by the Schrödinger-Newton equations. Using a Gaussian variational solution for the self-gravitating wave packet, combined with Nelson's stochastic representation of quantum dynamics, we track the evolution of particle ensembles whose initial probability distribution differs from $|Ψ|^2$. Relaxation to the Born rule ("quantum equilibrium") occurs when the wave packet remains bounded, or grows sufficiently slowly in time; in contrast, for rapidly expanding solutions of the Schrödinger-Newton equations, deviations from the Born rule can persist indefinitely. Numerical simulations confirm this analytical picture. These results show that semiclassical self-gravity can either enable or inhibit relaxation towards the Born rule, providing a minimal model relevant to proposals of primordial quantum non-equilibrium, as suggested by Underwood and Valentini [Phys. Rev. D 92, 063531 (2015)].

论文原文

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