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 paper introduces an eccentricity evolution consistency test (EECT) to distinguish true eccentric gravitational-wave signals from mimickers caused by other effects, improving the reliability of eccentric CBC detection.
Contribution
The paper proposes a novel method, EECT, that compares eccentricity evolution with frequency to confirm or reject eccentricity hypotheses in gravitational-wave signals.
Findings
EECT can reject mimickers at ≥68% confidence.
The method correctly identifies truly eccentric signals.
Demonstrated effectiveness with simulated CBC systems.
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).…
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Taxonomy
TopicsPulsars and Gravitational Waves Research
