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Re: value of g in black holes



Hi John-
I repeat, now that you seem to be on the verge of seeing the
light (or, perhaps, the black), what is the escape velocity from just
inside of the event horizon?
Regards,
Jack


On Thu, 18 Oct 2001, John Mallinckrodt wrote:

On Thu, 18 Oct 2001, Vic Decarlo wrote:

Perhaps John M., in speaking of a "completely
negligible" value of g at the event horizon of a very
massive black hole, is referring to relative tidal
accelerations for an observer radially plunging into
the black hole.

Yes and no. Although the tidal accelerations at the event horizon
clearly do diminish to negligible levels as M approaches the mass
of the universe, I was being more naive than that and using the
same sort of nonrelativistic--and, therefore, likely
incorrect--analysis that Carl Mungan had put forth and disclaimed.
I should have indicated my own discomfort with the analysis as
well since I'm not even sure how to interpret the concept of "g"
at an event horizon for reasons that were alluded to by Jack
Uretsky in his post. After all the value of g is normally
associated with observations that would be made by a "stationary"
observer--i.e., one who stays at constant R.

At any rate I am not surprised to learn that the relativistically
correct value diverges as one approaches the event horizon
regardless of M. I do wish, however, that I understood a little
better what that *meant*!

John Mallinckrodt mailto:ajm@csupomona.edu
Cal Poly Pomona http://www.csupomona.edu/~ajm


--
Franz Kafka's novels and novella's are so Kafkaesque that one has to
wonder at the enormity of coincidence required to have produced a writer
named Kafka to write them.
Greg Nagan from "The Metamorphosis" in
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