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Radial motion into an Einstein-Rosen bridge · Around

2009

Radial motion into an Einstein-Rosen bridge

Poplawski, Nikodem J.

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We consider the radial geodesic motion of a massive particle into a black hole in isotropic coordinates, which represents the exterior region of an Einstein-Rosen bridge (wormhole).

The particle enters the interior region, which is regular and physically equivalent to the asymptotically flat exterior of a white hole, and the particle's proper time extends to infinity.
Since the radial motion into a wormhole after passing the event horizon is physically different from the motion into a Schwarzschild black hole, Einstein-Rosen and Schwarzschild black holes are different, physical realizations of general relativity.
Yet for distant observers, both solutions are indistinguishable.

Built on

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