Fate of the first traversible wormhole: black-hole collapse or inflationary expansion
Hisa-aki Shinkai, Sean A. Hayward

TL;DR
This study numerically investigates the stability of Morris & Thorne's traversible wormhole, revealing its tendency to either collapse into a black hole or expand into an inflationary universe under perturbations, with implications for space-time foam.
Contribution
It demonstrates the instability of the first traversible wormhole solution and explores the conditions leading to black-hole formation or inflationary expansion, confirming a duality between wormholes and black holes.
Findings
Wormholes are unstable against Gaussian pulses in Klein-Gordon fields.
Perturbations lead to either black-hole collapse or inflationary expansion.
Critical solutions exhibit universal collapse times related to initial energy.
Abstract
We study numerically the stability of Morris & Thorne's first traversible wormhole, shown previously by Ellis to be a solution for a massless ghost Klein-Gordon field. Our code uses a dual-null formulation for spherically symmetric space-time integration, and the numerical range covers both universes connected by the wormhole. We observe that the wormhole is unstable against Gaussian pulses in either exotic or normal massless Klein-Gordon fields. The wormhole throat suffers a bifurcation of horizons and either explodes to form an inflationary universe or collapses to a black hole, if the total input energy is respectively negative or positive. As the perturbations become small in total energy, there is evidence for critical solutions with a certain black-hole mass or Hubble constant. The collapse time is related to the initial energy with an apparently universal critical exponent. For…
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