Local Structure of Numerically Generated Worm Hole Spacetime

TL;DR

This paper studies how the apparent horizons in a numerically simulated wormhole spacetime evolve, influenced by matter dynamics, and interprets these changes using the system's local mass.

Contribution

It introduces a detailed analysis of apparent horizon evolution in wormhole spacetimes through numerical simulation and local mass interpretation.

Findings

Apparent horizons are affected by matter field dynamics.

Local mass provides insight into wormhole structure evolution.

Numerical methods effectively track horizon behavior.

Abstract

We investigate the evolution of the apparent horizons in a numerically gererated worm hole spacetime. The behavior of the apparent horizons is affected by the dynamics of the matter field. By using the local mass of the system, we interpret the evolution of the worm hole structure. Figures are available by mail to author.