We argue that all dynamical astrophysical black hole merger channels are expected to result in a common eccentricity distribution at gravitational wave (GW) frequencies relevant for LIGO/Virgo/KAGRA (LVK) in the high eccentricity limit. This follows from the large separation of scales between the GW regime required for creating eccentric mergers in LVK, and the underlying astrophysical formation environment. Our analytical solution shows exceptional agreement with numerical studies. This finding has important implications for both theoretical studies and ongoing searches for eccentric GW sources.
@article{arxiv.2602.20110,
title = {The Universal Eccentricity Distribution for Dynamical Gravitational-Wave Merger Channels},
author = {Mor Rozner and Teagan A. Clarke and Isobel M. Romero-Shaw and Johan Samsing},
journal= {arXiv preprint arXiv:2602.20110},
year = {2026}
}