ClamShell
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Chalnoth said:...because the important quantities here are ones that are independent of the choice of coordinate system. For instance, if we take a path of an object that comes out from infinity and strikes the black hole, it spends an infinite amount of proper time outside the black hole traveling towards it, but once it reaches the event horizon, it takes a finite amount of proper time to strike the singularity. That sort of behavior is about as asymmetric as you can get.
My question was:
"...is the coordinate system on
our side of the event horizon in any way symmetrical with
the coordinate system chosen for the other side of the
event horizon? I am looking for symmetries that imply
conservation of entropy, as always."
My question is now:
Then it would seem to me that the Schwarzschild metric
(a metric now means to me; a tool for modeling a system,
on some underlying manifold, containing many particles,
many motions, and many observers)
...that the Schwarzschild metric transforms infinities
into finities as the BH horizon is crossed. Would it
not be more elegant for it to conserve (cleverly), the
time and space infinities on both sides of the horizon?
IE, if the horizon was just a regular curtain, the above
object would be free to continue its journey to another
(possibly different) infinity? Or, if the BH horizon is
really very exotic, to transform the above infinities
into into an infinite trajectory on the inside of the
event horizon?
No personal theory here...I just want entropies to balance.