  Understanding the late-time acceleration of the universe and its subtleties
is one of the biggest mysteries in cosmology. A lot of different approaches
have been put forward to deal with this, ranging from the conventional
cosmological constant to various models of dark energy and beyond. Recently one
very interesting approach to explaining the late time acceleration has been put
forward, where the the expansion of the universe is driven by mergers with
other "baby" universes and has been shown to be quite viable as well from the
point of view of recent observational data. So in this work we examine the
possibility of various rip scenarios and other future cosmological
singularities in such "multiversal" scenario, probing such singularities for
the first time in a multi universe scenario. We examine two models of such a
baby universe merging cosmology, and show that remarkably no rip scenario or
future cosmological singularity is possible in such models.
