It's ironic when a piece of writing tries to present you with factual information begins with a deceiving title, all in the name of attention grabbing.
Suppose there is a force F between masses M and m, separated by a distance r of the form F = Mmf(r) such that any spherically symmetric body affects external bodies as if its mass were concentrated at its centre. Then what form can the function f take?
The form of f allows Newtonian gravity but not Einsteinian.
[1] http://en.wikipedia.org/wiki/Shell_theorem#Converses_and_gen...
But the accretion disk might appear visible to various instruments.
Basically, we will see the exact location of the black hole for the first time directly. Not the collapsar itself, of course, but the swirling disk surrounding it.
In either case, the energy emissions potentially are enough, if they're directed at us and strong enough.