  In this manuscript we examine the Unruh-thermalized CERN-NA63 radiation
reaction data set from the point of view of a diphoton Rindler bath. Under the
assumption that these Hawking-Unruh diphoton pairs are microscopic
trans-Planckian black holes, we find the resultant heat capacity describes the
measured energy spectrum and is thus a dual description of the data set. Then,
employing an n-dimensional Stefan-Boltzmann analysis, we find the power
radiated by a black hole in the standard 3+1 spacetime dimensions in complete
agreement with the data. Finally, we utilize this power spectrum to directly
measure Newtons constant of gravitation.
