  The 2015 Planck data release has placed tight constraints on the allowed
class of inflationary models. The current data favors concave downwards
inflationary potentials while offering interesting hints on possible deviations
from the standard picture of CMB perturbations. We here test the predictions of
the theory of the origin of the universe from the landscape multiverse, against
the most recent Planck data, for the case of concave downwards inflationary
potentials, such as the Starobinsky model of inflation. By considering the
quantum entanglement correction of the multiverse, we can place a lower limit
on the local 'SUSY breaking' scale $b>1.2\times10^7 GeV$ at $95 \%$ c.l. from
Planck TT+lowTEB. We find that this limit is consistent with the range for $b$
that allows the landscape multiverse to explain a serie of anomalies present in
the current data.
