Testing Dark Energy with Black Hole Ringdown

Fuente: arXiv
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Auteurs principaux: Smulders, Laurens, Noller, Johannes, Sirera, Sergi
Format: Preprint
Publié: 2026
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author Smulders, Laurens
Noller, Johannes
Sirera, Sergi
author_facet Smulders, Laurens
Noller, Johannes
Sirera, Sergi
contents We show that dynamical dark energy theories can imprint $O(1)$ modifications on the quasi-normal mode (QNM) spectrum characterising black hole ringdown. The time dependence of dynamical dark energy naturally gives rise to cosmological 'hair' around a black hole. Taking the cubic Galileon as a concrete example, which admits the only known stable solution of this kind, we parametrically connect the cosmological and black hole regimes, derive the induced QNM shifts and forecast the resulting dark energy constraints. We find that the dark energy field profile can be constrained with an accuracy of up to $10^{-2}$ for LVK and $10^{-4}$ for LISA.
format Preprint
id arxiv_https___arxiv_org_abs_2603_23634
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle Testing Dark Energy with Black Hole Ringdown
Smulders, Laurens
Noller, Johannes
Sirera, Sergi
General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
We show that dynamical dark energy theories can imprint $O(1)$ modifications on the quasi-normal mode (QNM) spectrum characterising black hole ringdown. The time dependence of dynamical dark energy naturally gives rise to cosmological 'hair' around a black hole. Taking the cubic Galileon as a concrete example, which admits the only known stable solution of this kind, we parametrically connect the cosmological and black hole regimes, derive the induced QNM shifts and forecast the resulting dark energy constraints. We find that the dark energy field profile can be constrained with an accuracy of up to $10^{-2}$ for LVK and $10^{-4}$ for LISA.
title Testing Dark Energy with Black Hole Ringdown
topic General Relativity and Quantum Cosmology
Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
url https://arxiv.org/abs/2603.23634