Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers

Eccentric compact binary coalescences (CBCs) are expected to be observed in current and future gravitational-wave (GW) detector networks. Such detections are especially valuable as they can provide insights on the environments that nurture CBCs. 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. The standard approach to ascertain that a detected CBC is eccentric is to employ Bayesian model selection, where the eccentric CBC hypothesis is compared against other hypotheses. Such an approach is not only computationally intensive and time-consuming, but could also be misleading if none of the models under consideration represent the true model. 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 nonzero values of eccentricity, at some reference frequency, could be acquired when a noneccentric CBC with additional physical/beyond-GR effects is recovered with an eccentric CBC waveform model, the 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, quasicircular 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 $\ensuremath{\ge}68%$ confidence, while ensuring that truly eccentric CBCs satisfy EECT.

Authors

Institutions

Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-11-13
DOI
https://doi.org/10.1103/rstg-6n6y
Citations
1
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
1.15
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers

S. J. Kapadia, Avinash Tiwari, Md Arif Shaikh, Sajad A. Bhat
1 citations
Physical review. D/Physical review. D.
Pulsars and Gravitational Waves Research
1.15
article

Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers

S. J. Kapadia, Avinash Tiwari, Md Arif Shaikh, Sajad A. Bhat
article en
1 citations

Abstract

Eccentric compact binary coalescences (CBCs) are expected to be observed in current and future gravitational-wave (GW) detector networks. Such detections are especially valuable as they can provide insights on the environments that nurture CBCs. 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. The standard approach to ascertain that a detected CBC is eccentric is to employ Bayesian model selection, where the eccentric CBC hypothesis is compared against other hypotheses. Such an approach is not only computationally intensive and time-consuming, but could also be misleading if none of the models under consideration represent the true model. 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 nonzero values of eccentricity, at some reference frequency, could be acquired when a noneccentric CBC with additional physical/beyond-GR effects is recovered with an eccentric CBC waveform model, the 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, quasicircular 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 $\ensuremath{\ge}68%$ confidence, while ensuring that truly eccentric CBCs satisfy EECT.

Physical review. D/Physical review. D.Vol. 112(12)
Kanya Maha Vidyalaya (IN), Inter-University Centre for Astronomy and Astrophysics (IN)
Openalex Percentile: Top 15%
Pulsars and Gravitational Waves Research
1.15
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.