Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
Sajad A. Bhat, Avinash Tiwari, Md Arif Shaikh, Shasvath J. Kapadia
TL;DR
This work tackles the challenge of distinguishing truly eccentric gravitational-wave signals from eccentricity mimickers that arise from other physical or beyond-GR effects. It introduces the eccentricity Evolution Consistency Test (EECT), which tests GR-consistent eccentric evolution by comparing eccentricities recovered at a low reference frequency to those inferred at higher frequencies after evolving under GR, thereby avoiding exhaustive model comparisons. In a proof-of-concept with zero noise and an O4-like detector network, EECT rejects mimickers with ≥68% confidence while preserving genuine eccentric signals, across multiple mimicker scenarios including microlensing, LOSA, massive graviton, and dipole radiation. The approach leverages a 3PN GR eccentricity evolution and Bayesian parameter estimation to provide a robust, scalable discriminator for eccentricity in current and future GW observations. Its practical relevance grows with improved bandwidth and sensitivity, and future work will extend EECT to higher harmonics, spin effects, and more complex detector networks.
Abstract
Eccentric compact binary coalescences (CBCs) are expected to be observed in current and future gravitational-wave (GW) detector networks. However, it has been recently pointed out that a number of other physical and beyond-GR effects, could imitate, or be mimicked by, eccentric CBCs. In this work, we propose a conceptually simple but powerful method to directly confirm or reject the eccentric hypothesis, without needing to compare the hypothesis with the plethora of other possible hypotheses. The key idea is that while spurious non-zero values of eccentricity, at some reference frequency, could be acquired when a non-eccentric CBC with additional physical/beyond-GR effects is recovered with an eccentric CBC waveform model, the {\itshape evolution} of eccentricity with frequency will in general not be mimicked. We accordingly formulate an eccentricity evolution consistency test (EECT). The method compares the eccentricity recovered at some low frequency value (e.g, $10$ Hz), evolved to higher frequencies assuming GR, with eccentricities recovered at those same higher frequencies. Discrepancy between the two eccentricities at any reference frequency would violate EECT and indicate the presence of a mimicker. As a proof of concept, assuming a few eccentric CBC systems, quasi-circular CBCs with additional physics mimicking eccentricity, and an O4-like three-detector-network configuration, we demonstrate that our proposed method is indeed able to reject mimickers at $\geq 68\%$ confidence, while ensuring that truly eccentric CBCs satisfy EECT.
