Abstract
The possibility has been recently demonstrated to manufacture (nonrelativistic, Hamiltonian) many-body problems which feature an isochronous time evolution with an arbitrarily assigned period yet mimic with good approximation, or even exactly, any given many-body problem (within a quite large class, encompassing most of nonrelativistic physics) over times which may also be arbitrarily large (but of course such that ). In this paper we review and further explore the possibility to extend this finding to a general relativity context, so that it becomes relevant for cosmology.
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