论文标题
与互动的相对论GRW闪存过程
A Relativistic GRW Flash Process With Interaction
论文作者
论文摘要
在2004年，我描述了n不相互区分粒子的自发波函数崩溃的Ghirardi-Rimini-Weber（GRW）模型的相对论版本。在这里，我为N相互作用的可区分粒子提供了广义版本。目前，我不知道如何为无法区分的粒子或可变数量的粒子建立类似的模型。当前的相互作用模型是由给定的相互作用的统一的Tomonaga-Schinginging类型的型号构成的，插入了离散倒塌的空格曲面之间。我认为这种统一的进化是相互作用的本地（即，在间距分离时没有相互作用）。该模型是根据贝尔的闪光本体论提出的，但也与Ghirardi的物质密度本体论兼容。它是非本地的，并且满足了微观参数独立性和无信号。它也可以在弯曲的时空工作；在非相关主义极限中，它减少了已知的非忠实GRW模型。
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.
