Black Hole Interiors as a Laboratory for Time-Dependent Classical Double Copy
Damien A. Easson, Tucker Manton

TL;DR
This paper demonstrates that black hole interior regions, especially trapped Kerr--Schild geometries, serve as exact, time-dependent settings for the classical double copy correspondence between gravity and gauge theory.
Contribution
It establishes that trapped black hole interiors can be used as a local, exact laboratory for studying time-dependent classical double copy, including explicit examples like Bardeen and Schwarzschild solutions.
Findings
Bardeen solution yields a finite, regular single-copy field inside the trapped region.
Schwarzschild's single-copy electric field diverges during interior evolution.
Bardeen horizon phase structure is encoded in the single-copy scalar.
Abstract
The classical double copy provides a powerful bridge between gravity and gauge theory, but its most explicit realizations remain concentrated in stationary or highly symmetric settings. We show that trapped regions of black-hole geometries furnish an exact setting for time-dependent classical double copy. In the static, spherically symmetric case, each trapped interval admits a local single-copy description on the associated Kantowski--Sachs patch that is intrinsically time dependent, although it can be derived from static Kerr--Schild data and does not require knowledge of any exterior black-hole completion. We prove that this class is characterized intrinsically by a distinguished relation between the Kantowski--Sachs scale factors, equivalently by the longitudinal relation \(p_{\parallel}=-\rho\), and that the Kerr--Schild scalar and single-copy field are uniquely reconstructible…
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