A warp drive with predominantly positive invariant energy density and global Hawking-Ellis Type I
Jos\'e Rodal

TL;DR
This paper introduces a new warp-drive spacetime model within General Relativity that minimizes negative energy requirements and maintains a globally Type I stress-energy tensor, achieved through irrotational, curl-free kinematics.
Contribution
It provides the first explicit, continuous warp-drive solution with reduced negative energy and globally Type I stress-energy, emphasizing irrotational flow and detailed eigenanalysis.
Findings
Peak proper-energy deficit reduced by factors of 38 and 2600 compared to previous models.
Negative-energy volume is minimized, with net proper energy consistent with zero.
Solution maintains regularity at the origin and exhibits globally Type I stress-energy tensor.
Abstract
We present the first fully explicit, continuous, analytically derived warp-drive spacetime within General Relativity whose shift-vector flow is kinematically irrotational. Building on Santiago \emph{et al.} that scalar-potential, zero-vorticity warp fields are Hawking-Ellis Type I for unit lapse and flat spatial slices, we supply a closed-form scalar potential and smooth shift components with proper boundary behavior, together with a Cartan-tetrad analytic pipeline and high-precision eigenanalysis. Compared with the Alcubierre and Nat\'{a}rio models (evaluated at identical parameters ), our irrotational solution exhibits \emph{significantly reduced} local NEC/WEC stress: its peak proper-energy deficit is reduced by a factor of relative to Alcubierre and relative to Nat\'{a}rio, and its peak NEC violation is more than $60…
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Taxonomy
TopicsCosmology and Gravitation Theories · Quantum Electrodynamics and Casimir Effect · Black Holes and Theoretical Physics
