Infall time in the Eddington-Finkelstein metric, with application to Einstein-Rosen bridges
Abstract
The Eddington-Finkelstein metric is obtained from the Schwarzschild metric by a change of the time variable. It is well known that a test mass falling into a black hole does not reach the event horizon for any finite value of the Schwarzschild time variable . By contrast, we show that the event horizon is reached for a finite value of the Eddington-Finkelstein time variable . Then we study in Eddington-Finkelstein time the fate of a massive particle traversing an Einstein-Rosen bridge and obtain a different conclusion than recent proposals in the literature: we show that the particle reaches the wormhole throat for a finite value of the time marker , and continues its trajectory across the throat for . Such a behavior does not make sense in Schwarzschild time since it would amount to continuing the trajectory of the particle "beyond the end of time."
Keywords
Cite
@article{arxiv.2110.05938,
title = {Infall time in the Eddington-Finkelstein metric, with application to Einstein-Rosen bridges},
author = {Pascal Koiran},
journal= {arXiv preprint arXiv:2110.05938},
year = {2021}
}
Comments
To appear in International Journal of Modern Physics D