A Stochastic Open-System Boundary Effective Field Theory for Late-Time Gravitational-Wave Relaxation

We construct a mathematically controlled, open-system boundary effective field theory (EFT) to model the late-time stochastic residual response in post-merger gravitational-wave spectroscopy. While deterministic strong-field merger dynamics remain strictly governed by the classical Einstein field equations, integrating out unresolved high-energy degrees of freedom at a timelike matching hypersurface exterior to the horizon generates a non-local boundary effective action. Using a linear spin-2 tensor sourcing framework where asymptotic gravitational perturbations couple to a primary boundary conformal field theory (bCFT) operator , we derive a non-local, dissipative mixed Robin boundary condition from variational stationarity of the coupled bulk-boundary action. We demonstrate a fundamental structural bifurcation within the induced self-energy loop integral: all ultraviolet-sensitive, regulator-dependent contributions are strictly polynomial and local in the time domain, allowing their systematic order-by-order absorption into a standard tower of local boundary counterterms . Conversely, analytic continuation of the infrared scale-invariant sector generates a universal, regulator-independent continuum response sector parameterized by the fundamental scaling dimension . Choosing the principal branch such that the non-meromorphic cut lies entirely along the negative imaginary frequency axis satisfies Titchmarsh’s theorem, guarantees causality in the upper half-plane, and ensures immunity to Ostrogradsky or runaway instabilities. Imposing simultaneous constraints from Kramers–Kronig contour convergence and spectral positivity establishes a derived conformal stability window 1.5 < \Delta_{\mathcal O} < 3.5. Finally, utilizing the fluctuation-dissipation relation, we project the continuum spectral density into a structured non-local metric covariance operator \mathbf{\Gamma}(\Delta_{\mathcal O},\mathcal G_B,\theta), The present framework should be interpreted as a phenomenological open-system EFT constrained by causality, renormalizability, and infrared scaling consistency.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-05-18
DOI
https://doi.org/10.5281/zenodo.20271754
Primary Topic
Pulsars and Gravitational Waves Research
Type
preprint
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preprint

A Stochastic Open-System Boundary Effective Field Theory for Late-Time Gravitational-Wave Relaxation

John Strother
Zenodo (CERN European Organization for Nuclear Research)
Pulsars and Gravitational Waves Research
preprint

A Stochastic Open-System Boundary Effective Field Theory for Late-Time Gravitational-Wave Relaxation

John Strother
preprint en

Abstract

We construct a mathematically controlled, open-system boundary effective field theory (EFT) to model the late-time stochastic residual response in post-merger gravitational-wave spectroscopy. While deterministic strong-field merger dynamics remain strictly governed by the classical Einstein field equations, integrating out unresolved high-energy degrees of freedom at a timelike matching hypersurface exterior to the horizon generates a non-local boundary effective action. Using a linear spin-2 tensor sourcing framework where asymptotic gravitational perturbations couple to a primary boundary conformal field theory (bCFT) operator , we derive a non-local, dissipative mixed Robin boundary condition from variational stationarity of the coupled bulk-boundary action. We demonstrate a fundamental structural bifurcation within the induced self-energy loop integral: all ultraviolet-sensitive, regulator-dependent contributions are strictly polynomial and local in the time domain, allowing their systematic order-by-order absorption into a standard tower of local boundary counterterms . Conversely, analytic continuation of the infrared scale-invariant sector generates a universal, regulator-independent continuum response sector parameterized by the fundamental scaling dimension . Choosing the principal branch such that the non-meromorphic cut lies entirely along the negative imaginary frequency axis satisfies Titchmarsh’s theorem, guarantees causality in the upper half-plane, and ensures immunity to Ostrogradsky or runaway instabilities. Imposing simultaneous constraints from Kramers–Kronig contour convergence and spectral positivity establishes a derived conformal stability window 1.5 < \Delta_{\mathcal O} < 3.5. Finally, utilizing the fluctuation-dissipation relation, we project the continuum spectral density into a structured non-local metric covariance operator \mathbf{\Gamma}(\Delta_{\mathcal O},\mathcal G_B,\theta), The present framework should be interpreted as a phenomenological open-system EFT constrained by causality, renormalizability, and infrared scaling consistency.

Zenodo (CERN European Organization for Nuclear Research)
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Pulsars and Gravitational Waves Research
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A Stochastic Open-System Boundary Effective Field Theory for Late-Time Gravitational-Wave Relaxation — John Strother · Zenodo (CERN European Organization for Nuclear Research) (2026) | TGRS Research Map | TGRS