25-AUG-2007
Hi all -
Assuming, for the sake of simplicity, a non-rotating BH, it's been
conjectured that for an external observer the "image" of any matter
falling through the critical circumference is (forever) frozen at the
horizon. Two questions:
1. Doesn't this essentially preserve (some) information about the
infalling matter, for any external observer, and
2. Doesn't this endow the BH with hair?
The idea seems to suggest that any BH that has ingested matter would
have a horizon forever postered with the images of these hapless bits,
for any passing observer to see. How then would the black hole remain
dark to the outside universe?
cheers,
mark jonathan horn
Bran - 27 Aug 2007 07:44 GMT
Hi!
> Assuming, for the sake of simplicity, a non-rotating BH, it's been
> conjectured that for an external observer the "image" of any matter
[quoted text clipped - 10 lines]
> for any passing observer to see. How then would the black hole remain
> dark to the outside universe?
1. No. Because there is no way to access such information (from outside
the black hole). For instance if some sort of transmitter approaches BH
horizon the signal intensity exponentially decays as that transmitter
approaches horizon (See, for instance, problem (and solution) #15.10 in
``Problem Book in Relativity and Gravitation'' by Lightman et al.), the
time constant in such an exponent is of order R_h/c.
There is also no way to ``lit up'' the matter ``postered'' on the
horizon because the ``light'' one could use to do that will not catch up
with the such matter before it enters the horizon.
2. Various ``no-hair'' assertions for black holes do not prohibit the
existence of such perturbations around black holes. But such
perturbations either decay rapidly or are radiated away, leaving black
hole itself without any ``hairs''.
WBR,

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