  We revisit the construction of models of quantum gravity in d dimensional
Minkowski space in terms of random tensor models, and correct some mistakes in
our previous treatment of the subject. We find a large class of models in which
the large impact parameter scattering scales with energy and impact parameter
like Newton`s law. These same models also have emergent energy, momentum and
angular conservation laws, despite being based on time dependent Hamiltonians.
Many of the scattering amplitudes have a Feynman diagram like structure: local
interaction vertices connected by propagation of free particles (really
Sterman-Weinberg jets of particles). However, there are also amplitudes where
jets collide to form large meta-stable objects, with all the scaling properties
of black holes: energy, entropy and temperature, as well as the characteristic
time scale for the decay of perturbations. We generalize the conjecture of
Sekino and Susskind, to claim that all of these models are fast scramblers. The
rationale for this claim is that the interactions are invariant under fuzzy
subgroups of the group of volume preserving diffeomorphisms, so that they are
highly non-local on the holographic screen. We review how this formalism
resolves the Firewall Paradox.
