- #351
A.T.
Science Advisor
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An interesting intuitive approach for this problem is presented by Epstein in his book "Relativity Visalized". He uses space-propertime embeddings of the Schwarzshild-Metric like this one:
http://www.adamtoons.de/physics/gravitation.swf
"space" : radial Schwarzshild coordinate r
"proper time" : the proper time elapsed along the cyan world line
length of the world line : Schwarzshild coordinate time t
inflation of the "pipe" at certain r : time dialtion of a static clock at that r relative to t
For a BH the funnel would inflate infinitely into a plateau at the event horizon:
The cyan world line here can have an infinite length (coordinate time t) but will still cover a finite angular displacement around the pipe (proper time)