A warp drive with predominantly positive invariant energy density and global Hawking-Ellis Type I

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 Natário models (evaluated at identical parameters $\rho ,\sigma ,v\mathrm{/}c$), our irrotational solution exhibits \emph{significantly reduced} local NEC/WEC stress: its peak proper-energy deficit is reduced by a factor of $\approx 38$ relative to Alcubierre and $\approx 2.6\times {10}^3$ relative to Natário, and its peak NEC violation is more than $60\times$ smaller than Natário. Crucially, the stress-energy is \emph{globally} Hawking-Ellis Type I, with a well-defined timelike eigenvalue (proper energy density) everywhere. A fixed-smoothing vortical ablation confirms that this improvement is causally due to irrotational, curl-free kinematics rather than profile shaping: adding modest vorticity collapses the $E_{+}\mathrm{/}{E}_{-}$ balance and drives large increases in the negative-energy magnitude $E_{-}$. We quantify the negative-energy requirement via a \emph{slice-integrated} (on ${\mathrm{\Sigma }}_t$) negative-energy volume and tabulate global measures. A far-field extrapolation to $R\to \mathrm{\infty }$ yields tail-corrected totals $\mathrm{\mid }{E}_{+}-E_{-}\mathrm{\mid }\mathrm{/}(E_{+}+E_{-})=0.04\mathrm{\%}$. Thus the net \emph{proper} energy is consistent with zero to four decimal places (in fractional units). We also establish regularity at $r=0$ for the irrotational construction.