  A Multiverse can arise from landscapes without de Sitter minima. It can be
populated during a period of eternal inflation without trans-Planckian field
excursions and without flat potentials. This Multiverse can explain the values
of the cosmological constant and of the weak scale. In the process of proving
these statements we derive a few simple, but counter-intuitive results. We show
that it is easy to write models of eternal inflation compatible with the
distance and refined de Sitter conjectures. Secondly, tunneling transitions
that move fields from a lower-energy vacuum to a higher-energy vacuum and
generate baby Universes are possible, and occur during eternal inflation.
Finally, we relax the assumption of no de Sitter minima and show that this more
standard Multiverse can be populated by Coleman-De Luccia transitions in about
100 $e$-folds of inflation.
