Closed timelike curves in PT-symmetric wormholes
Hicham Zejli

TL;DR
This paper introduces a PT-symmetric wormhole model with unidirectional traversability, enabling the formation of closed timelike curves and analyzing scalar field dynamics within this novel spacetime framework.
Contribution
It presents a new PT-symmetric bimetric wormhole model that allows CTCs and explores scalar field behavior, extending the understanding of causality in such geometries.
Findings
PT-symmetric wormhole model with traversability
Generation of closed timelike curves via coupled wormholes
PT-symmetric Klein-Gordon equations with real spectra
Abstract
We investigate a modified Einstein-Rosen wormhole model, made unidirectionally traversable through a bimetric geometry defined by two regular metrics, g(+) and g(-), and characterized by PT symmetry combining time reversal (t -> -t) and spatial inversion (x -> -x). In this framework, two distinct spacetime regions are identified at the wormhole throat (r = alpha) via PT symmetry, forming a single spacetime sheet. This model employs Eddington-Finkelstein coordinates to eliminate coordinate singularities at the throat, enabling traversability with a lightlike membrane of exotic matter at the junction to satisfy the Einstein field equations, similar to other traversable wormhole models. We extend this model by coupling two such wormholes to generate closed timelike curves (CTCs), made possible by the opposing causal orientations defined by the two metrics, while adhering to Novikov's…
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