Spacetime topology from the tomographic histories approach I: `Classical' Case
I. Raptis, Petros Wallden, Romàn R. Zapatrin
The tomographic histories approach is presented. As an inverse problem, we recover in an operational way the effective topology of the extended configuration space of a system. This means that from a series of experiments we get a set of points corresponding to events. The difference between effective and actual topology is drawn. We deduce the topology of the extended configuration space of a ‘classical ’ (i.e. non-relativistic) system, using certain concepts from the consistent histories approach to Quantum Mechanics, such as the notion of a record. A few remarks about the case of a relativistic system, preparing the ground for a forthcoming paper sequel to this, are made in the end. 1 Introduction with Motivational Remarks In the standard formulation of relativity theory, the spacetime topology is a priori fixed by the theorist to that of a continuous manifold; hence, it is not an observable entity. Only the metric structure is traditionally supposed to be dynamically variable. With the exception of Wheeler’s celebrated, but largely heuristic, spacetime foam scenario
•Jun 16, 2005•0 citations