Passing the Einstein-Rosen bridge

Abstract

We relax the requirement of geodesic completeness of a space-time. Instead, we require test particles trajectories to be smooth only in the physical sector. Test particles trajectories for Einstein--Rosen bridge are proved to be smooth in the physical sector, and particles can freely penetrate the bridge in both directions.

6 pages, 2 figures

References in corpus (3)

• Radial motion into an Einstein-Rosen bridge
• Einstein-Rosen "Bridge" Needs Lightlike Brane Source
• Point massive particle in General Relativity

Cited by in corpus (6)

• Finite Action Principle and Horava-Lifshitz Gravity: early universe, black holes and wormholes
• Infall time in the Eddington-Finkelstein metric, with application to Einstein-Rosen bridges
• Torsional Elastic Waves in Double Wall Tube
• Finite Action Principle and wormholes
• Einstein-Rosen "Bridge" Revisited and Lightlike Thin-Shell Wormholes
• Kruskal-Penrose Formalism for Lightlike Thin-Shell Wormholes