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Pitching Cosmic Curveballs: Environmental Effects on Extreme-Mass-Ratio Inspirals with Spinning Secondaries

Leif Lui1, Lisa V. Drummond2, and Alejandro Torres-Orjuela1,*

  • *Contact author: atorreso@bimsa.cn

Phys. Rev. Lett. 137, 121403 – Published 16 September, 2026

DOI: https://doi.org/10.1103/dy3h-65ty

Abstract

Much like the aerodynamic deflection of a spinning curveball, a rotating secondary in an extreme-mass-ratio inspiral (EMRI) experiences Magnus and lift forces, in addition to the standard drag force, when traversing a gaseous environment. We present the first framework that incorporates these specific spin-coupled environmental effects (EEs) into the evolution of EMRI. Over the multiyear observation windows of space-based gravitational wave (GW) detectors, these interactions imprint a unique, distinguishable dephasing signature on the signal. Crucially, a Fisher matrix analysis reveals that gas drag breaks the fundamental vacuum-projection degeneracy between the secondary’s spin magnitude and inclination, thereby tightening parameter constraints. Thus, accounting for EEs is not merely a modeling necessity, but could potentially be a powerful tool for enhancing the detectability of the secondary’s intrinsic spin, and could serve as a novel probe of accretion flows harboring massive black holes.

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Article Text

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