Holographic Space-time, Newton's Law and the Dynamics of Black Holes

Understand

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).