  Recent work on the status of astrophysical modeling in the wake of quantum
gravity indicates that a 'fauxrizon' (portmanteau of 'faux horizon'), such as
is relevant to understanding astrophysical black holes according to the
fuzzball proposal within string theory, might ultimately solve the familiar
black hole evaporation paradox. I clarify, with general upshots for the
foundations of quantum gravity research, some of what this suggestion would
amount to: identification of intertheoretic constraints on global spacetime
structure in (observer-relative) semiclassical models of fuzzballs.
