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arXiv 2002.00482quant-ph
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一种带相互作用的相对论性GRW闪现过程

A Relativistic GRW Flash Process With Interaction

Roderich Tumulka

AI总结:

本文将GRW自发坍缩模型推广到N个相互作用可区分粒子的相对论情形,基于Tomonaga-Schwinger型幺正演化插入离散坍缩,并证明其满足无信号条件、适用于弯曲时空且在非相对论极限下约化为标准GRW模型。

摘要:

2004年,我描述了一种针对N个非相互作用可区分粒子的Ghirardi-Rimini-Weber(GRW)自发波函数坍缩模型的相对论版本。本文中,我提出一个针对N个相互作用可区分粒子的广义版本。目前,我尚不知道如何为不可区分粒子或粒子数可变的情况建立类似模型。本文的相互作用模型由一个给定的相互作用幺正Tomonaga-Schwinger型演化构造而成,该演化定义在类空超曲面之间,并在其中插入离散坍缩。我假设该幺正演化是相互作用局域的(即类空分离处无相互作用)。该模型以Bell的闪现本体论(flash ontology)表述,但也与Ghirardi的物质密度本体论(matter density ontology)相容。该模型是非局域的,且满足微观参数独立性和无信号(no-signaling)条件;它也适用于弯曲时空;在非相对论极限下,它约化为已知的非相对论GRW模型。

英文摘要:

In 2004, I described a relativistic version of the Ghirardi-Rimini-Weber (GRW) model of spontaneous wave function collapse for N non-interacting distinguishable particles. Here I present a generalized version for N interacting distinguishable particles. Presently, I do not know how to set up a similar model for indistinguishable particles or a variable number of particles. The present interacting model is constructed from a given interacting unitary Tomonaga-Schwinger type evolution between spacelike hypersurfaces, into which discrete collapses are inserted. I assume that this unitary evolution is interaction-local (i.e., no interaction at spacelike separation). The model is formulated in terms of Bell's flash ontology but is also compatible with Ghirardi's matter density ontology. It is non-local and satisfies microscopic parameter independence and no-signaling; it also works in curved space-time; in the non-relativistic limit, it reduces to the known non-relativistic GRW model.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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