Semiclassical instability of dynamical warp drives
Stefano Finazzi, Stefano Liberati, Carlos Barcel\'o

TL;DR
This paper investigates the semiclassical stability of dynamical warp drives in General Relativity, revealing that quantum effects cause exponential growth in stress-energy, leading to instability of the warp-drive spacetime.
Contribution
It extends previous analyses by studying the more realistic dynamical warp drives created from flat spacetime, and examines their quantum stability through the behavior of the renormalized stress-energy tensor.
Findings
Hawking radiation flux at the warp drive center
Exponential growth of stress-energy near the bubble front
Instability of warp-drive geometries due to semiclassical back-reaction
Abstract
Warp drives are very interesting configurations in General Relativity: At least theoretically, they provide a way to travel at superluminal speeds, albeit at the cost of requiring exotic matter to exist as solutions of Einstein's equations. However, even if one succeeded in providing the necessary exotic matter to build them, it would still be necessary to check whether they would survive to the switching on of quantum effects. Semiclassical corrections to warp-drive geometries have been analyzed only for eternal warp-drive bubbles traveling at fixed superluminal speeds. Here, we investigate the more realistic case in which a superluminal warp drive is created out of an initially flat spacetime. First of all we analyze the causal structure of eternal and dynamical warp-drive spacetimes. Then we pass to the analysis of the renormalized stress-energy tensor (RSET) of a quantum field in…
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