Gravitational Enstrophy: Local Geometric Origin and Energy-Cascade Constraints

arXiv:2608.03697 · gr-qc, astro-ph.HE, hep-th · Submitted 2026-08-04 · Read on arXiv

gr-qc, astro-ph.HE, hep-th

Submitted: 2026-08-04

Updated: 2026-10-05

Comments: 41 pages (1/2 are appendices for specific details), 3 figures [a few typos fixed, added a clarifying paragraph]

License: http://creativecommons.org/licenses/by-nc-nd/4.0/

The gist: Two-dimensional fluids conserve energy and enstrophy, driving inverse energy cascades via Fj rtoft's argument.

Terminology

Abstract

Two-dimensional fluids conserve energy and enstrophy, driving inverse energy cascades via Fj rtoft's argument. We show General Relativity admits an analogous structure: for linear radiative perturbations of Petrov type D backgrounds (Kerr, Kerr--AdS), the gravitational-wave energy W = sum k W k and magnetic Weyl enstrophy Z = integral B ab B ab sqrt gamma, d 3x about sum k omega k squared W k are approximately conserved in the zero-angular momentum frame, where vorticity coupling vanishes identically and curl exchange cancels mode-by-mode. This yields a gravitational Fj rtoft constraint implying nonlinear energy transfer proceeds preferentially toward lower frequencies. The constraint is dynamically active in near-extremal Kerr (tau damp tau nl) and confined geometries (AdS), but suppressed in generic ringdown. In AdS, Z maps holographically to the boundary fluid enstrophy.

Sources

Related papers