If, from far away, nothing gets inside a black hole, how do they accrete
and grow?
Matter does not have to fall
THROUGH the event horizon to make a black hole for outside observers. All it
has to do is get close enough to the horizon, by literally a few millimeters,
so that it experiences a large relativistic dilation factor. The emitted light
will be highly redshifted from gamma ray energies to radio wavelengths during
this last few millimeters, and as seen by an outside observer, the matter will
cease to emit light or energy. As seen by a distant observer, the object
accretes mass which falls towards its horizon limit...and then seems to slow
down and stop before 'winking out'.
Only to an infalling observer will the
matter actually be seen to pass across the horizon and fall into the
singularity, but this is not ever observable to the outside party in a finite
amount of time. Black holes are to general relativity what the Twin Paradox is
to special relativity.
Copyright 1997 Dr. Sten Odenwald
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