Ringdown modulation of acceleration radiation in the Schwarzschild background
Reggie C. Pantig

TL;DR
This paper analytically describes how black hole ringdown affects near-horizon thermality signatures, revealing a universal, decaying-oscillatory modulation linked to quasinormal modes, with implications for understanding black hole radiation.
Contribution
It introduces a gauge-invariant, analytic framework for understanding ringdown effects on near-horizon thermality, extending previous static models to include perturbations and dynamic signatures.
Findings
Ringdown causes a universal, decaying-oscillatory modulation of the Boltzmann exponent.
The response coefficient is derived explicitly at the sampling radius.
Near-horizon thermality remains robust despite ringdown perturbations.
Abstract
We present an analytic, first-order description of how black hole ringdown imprints on the operational signature of near-horizon thermality. Building on a static Schwarzschild baseline in which a freely falling two-level system coupled to a single outgoing mode exhibits geometric photon statistics and a detailed-balance ratio set by the surface gravity, we introduce an even-parity, axisymmetric quadrupolar perturbation and work in an ingoing Eddington-Finkelstein, horizon-regular framework. The perturbation corrects the outgoing eikonal through a gauge-invariant double-null contraction of the metric, yielding a compact redshift map that, when pulled back to the detector worldline, produces a universal, decaying-oscillatory modulation of the Boltzmann exponent at the quasinormal frequency. We derive a closed boundary formula for the response coefficient at the sampling radius, identify…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Relativity and Gravitational Theory
