Wednesday, April 14, 2010

Wormholes

From Poplawski we get:

"As the particle moves from infinity to r = rg /4, θ decreases from 0 to −3/(2rg ). At r = rg /4, θ undergoes a discontinuity, jumping to 3/(2rg ). As the particle moves from r = rg /4 to r = 0, θ decreases back to zero. The discontinuity of the expansion scalar at the event horizon of a wormhole prevents θ from decreasing to −∞, as it occurs inside a Schwarzschild black hole. Therefore this discontinuity guarantees that timelike geodesics in the gravitational field of a wormhole are complete."

This is the mathematics that goes with Frampton's solution to the Dark Energy Problem: There is no Dark Energy, because Gravity is not fundamental, and there is universal acceleration, because we are inside a black hole.

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