Rotation and twist regular modes for trapped ghosts

Abstract

A parameter-independent notion of stationary slow motion is formulated then applied to the case of stationary rotation of massless trapped ghosts. The excitations correspond to a rotation mode with angular momentum $J\ne 0$ and twist modes. It is found that the rotation mode, which has no parity, causes excess in the angular velocity of dragged distant coordinate frames in one sheet of the wormhole while in the other sheet the angular velocity of the ghosts is that of rotating stars: $2J/r^3$. As to the twist modes, which all have parity, they cause excess in the angular velocity of one of the throat's poles with respect to the other.

11 pages, 3 figures; General Relativity and Gravitation - 2012

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• Wormhole solutions sourced by fluids, II: Three-fluid two-charged sources
• Epicyclic oscillations of charged particles in stationary solutions immersed in a magnetic field with application to the Kerr--Newman black hole
• Wormhole solutions sourced by fluids, I: Two-fluid charged sources