ADM mass in warp drive spacetimes
Sebastian Schuster (Charles University of Prague), Jessica Santiago, (Aristotle University of Thessaloniki), and Matt Visser (Victoria University, of Wellington)

TL;DR
This paper rigorously analyzes the concept of mass in warp drive spacetimes, demonstrating that such spacetimes violate all classical energy conditions and clarifying misconceptions about the nature of mass and payloads in warp drives.
Contribution
It provides an exact, explicit computation of stress-energy components in warp drive spacetimes, clarifies the role of mass, and confirms violations of all classical energy conditions.
Findings
Warp drive spacetimes violate NEC, WEC, SEC, DEC.
Explicit stress-energy tensor calculations are provided.
Clarifies the distinction between bubble mass and background features.
Abstract
What happens when a warp bubble has mass? This seemingly innocent question forces one to carefully formalize exactly what one means by a warp bubble, exactly what one means by having the warp bubble "move" with respect to the fixed stars, and forces one to more carefully examine the notion of mass in warp-drive spacetimes. This is the goal of the present article. In this process, we will see that often-made throw-away comments regarding "payloads" are even simpler than commonly assumed, while there are two further, distinct yet subtle ways in which a mass can appear in connection with a warp drive space-time: One, that the warp bubble (not its payload) has the mass; two, that the mass is a background feature in front of which the warp drive moves. For simplicity, we consider generic Nat\'ario warp drives with zero-vorticity flow field. The resulting spacetimes are sufficiently simple to…
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Taxonomy
TopicsCosmology and Gravitation Theories · Solar and Space Plasma Dynamics · Computational Physics and Python Applications
