  We derive the Smarr formulae for two five-dimensional solutions of
supergravity, which are asymptotically R^(1,3)xS^1; in particular, one has a
magnetic bolt in its center, and one is a two-center solution. We show for both
spacetimes that supersymmetry - and so the BPS-bound - is broken by the
holonomy and how each topological feature of a space-like hypersurface enters
Smarr's mass formula, with emphasis on the ones that give rise to the stated
violation of the BPS-bound. In this light, we question if any violating
extra-mass term in a spacetime with such asymptotics is only evident in the ADM
mass while the Komar mass per se tries to preserve BPS. Finally, we derive the
cohomological fluxes for each situation and examine in a more general fashion
how the breaking of supersymmetry - and so the BPS-bound violation - is
associated with their topologies. In the second (and more complicated)
scenario, we especially focus on the compact cycle linking the centers, and the
contribution of non-vanishing bulk terms in the mass formula to the breaking of
supersymmetry.
