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title: "Signatures of Quantum Gravity in Gravitational Wave Memory" | ||
authors: | ||
- "Deppe, Nils" | ||
- "Heisenberg, Lavinia" | ||
- "Kidder, Lawrence E." | ||
- "Maibach, David" | ||
- "Ma, Sizheng" | ||
- "Moxon, Jordan" | ||
- "Nelli, Kyle C." | ||
- "Throwe, William" | ||
- "Vu, Nils L." | ||
jref: | ||
doi: | ||
date: 2025-02-27 | ||
arxiv: "2502.20584" | ||
used_spec: true | ||
abstract: | | ||
We study the impact of quantum corrections to gravitational | ||
waveforms on the gravitational wave memory effect. In certain | ||
quantum gravity theories and semi-classical frameworks, black holes | ||
(or other exotic compact objects) exhibit reflective properties that | ||
cause quasi-normal modes of a binary merger waveform to partially | ||
reflect off the horizon. If these reflections reach the detector, | ||
the measured gravitational wave signal may show echo-like features | ||
following the initial ringdown phase. Detecting such echoes, or | ||
their indirect signatures, would offer compelling evidence for the | ||
quantum nature of black holes. Given that direct detection of echoes | ||
requires finely tuned waveform templates, exploring alternative | ||
imprints of this phenomenon is crucial. In this work, we pursue this | ||
goal by calculating corrections to the null memory arising from | ||
echo-like features, formulated in terms of the Newman-Penrose scalar | ||
\(\Psi_0\). We demonstrate that the morphology of the resulting | ||
features is model-independent rendering them conceptually much | ||
easier to detect in real interferometer data than the raw echo. The | ||
corresponding signal-to-noise ratio of echo-induced features | ||
appearing in the gravitational wave memory is estimated | ||
subsequently. We further compute the physical fluxes associated to | ||
the echo at both the black hole horizon and null infinity and | ||
identify novel distinguishing features of the underlying | ||
reflectivity models in measurement data. | ||
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