On the Dynamical Formation of the Dyadosphere

Physics

Scientific paper

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Scientific paper

We discuss the evolution of the plasma around a collapsing star core endowed with a net electric charge described by the Reissner-Norstrorn geometry. The star is assumed to reach values of the electric field larger than the Heisenberg-Euler-Schwinger critical value for pair production. We consider the dynamical formation of the Dyadosphere. We show that the plasma near the event horizon falls into the black hole, while the outer plasma expands reaching ultrarelativistic velocities.

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