LIFETIMES OF SPHERICALLY SYMMETRICAL CLOSED UNIVERSES

It is proven that any spherically symmetric spacetime that possesses a compact Cauchy surface and that satisfies the dominant-energy and non-negative-pressure conditions must have a finite lifetime in the sense that all timelike curves in such a spacetime must have a length no greater than 10 max(2m), where m is the mass associated with the spheres of symmetry. This result gives a complete resolution, in the spherically symmetric case, of one version of the closed-universe recollapse conjecture (though it is likely that a slightly better bound can be established). This bound has the desirable properties of being computable from the (spherically symmetric) initial data for the spacetime and having a very simple form. In fact, its form is the same as was established, using a different method, for the spherically symmetric massless scalar field spacetimes, thereby proving a conjecture offered in that work. Prospects for generalizing these results beyond the spherically symmetric case are discussed. © 1995 The American Physical Society.