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 TT 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 T~\tilde{T} which may also be arbitrarily large (but of course such that T~<T\tilde{T}<T). 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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