  We discuss a remarkable correspondence between the description of Black Holes
as highly occupied condensates of $N$ weakly interacting gravitons and that of
Color Glass Condensates (CGCs) as highly occupied gluon states. In both cases,
the dynamics of "wee partons" in Regge asymptotics is controlled by emergent
semi-hard scales that lead to perturbative unitarization and classicalization
of $2\rightarrow N$ particle amplitudes at weak coupling. In particular, they
attain a maximal entropy permitted by unitarity, bounded by the inverse
coupling $\alpha$ of the respective constituents. Strikingly, this entropy is
equal to the area measured in units of the Goldstone constant corresponding to
the spontaneous breaking of Poincar{\'{e}} symmetry by the corresponding
graviton or gluon condensate. In gravity, the Goldstone constant is the Planck
scale, and gives rise to the Bekenstein-Hawking entropy. Likewise, in the CGC,
the corresponding Goldstone scale is determined by the onset of gluon
screening. We point to further similarities in Black Hole formation,
thermalization and decay, to that of the Glasma matter formed from colliding
CGCs in ultrarelativistic nuclear collisions, which decays into a Quark-Gluon
Plasma.
