Inflating wormholes in the braneworld models
K. C. Wong, T. Harko, K. S. Cheng

TL;DR
This paper explores how wormholes in braneworld models evolve during inflation, showing that some can grow or transform into black holes, with implications for understanding higher-dimensional gravity and cosmology.
Contribution
It investigates the evolution of inflating wormholes in braneworld scenarios, including embedding conditions, dynamics during inflation, and the potential transformation into black holes.
Findings
Wormholes can be supported by nonlocal brane effects without violating energy conditions.
During inflation, some wormholes decay, while others may become black holes.
A zero redshift wormhole solution was explicitly obtained.
Abstract
The braneworld model, in which our Universe is a three-brane embedded in a five-dimensional bulk, allows the existence of wormholes, without any violation of the energy conditions. A fundamental ingredient of traversable wormholes is the violation of the null energy condition (NEC). However, in the brane world models, the stress energy tensor confined on the brane, threading the wormhole, satisfies the NEC. In conventional general relativity, wormholes existing before inflation can be significantly enlarged by the expanding spacetime. We investigate the evolution of an inflating wormhole in the brane world scenario, in which the wormhole is supported by the nonlocal brane world effects. As a first step in our study we consider the possibility of embedding a four-dimensional brane world wormhole into a five dimensional bulk. The conditions for the embedding are obtained by studying the…
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