The membrane paradigm for a dynamic wormhole

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

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5 pages, no figures

Scientific paper

A classical membrane model is developed for a dynamic wormhole. Its throat
expands hyperbolically with an acceleration proportional to the surface energy
density $\sigma$. The model leads to a negative bulk viscosity coefficient
$\zeta = - 1/6 \pi$ on the throat, expressing the instability against
perturbations (expansions or contractions).

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