BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Eccentricity evolution consistency test to distinguish eccentric g
 ravitational-wave signals from eccentricity mimickers
DTSTART;VALUE=DATE-TIME:20260705T093000Z
DTEND;VALUE=DATE-TIME:20260705T094500Z
DTSTAMP;VALUE=DATE-TIME:20261027T091251Z
UID:indico-contribution-811@indico.narit.or.th
DESCRIPTION:Speakers: Sajad Ahmad Bhat (Inter-University Center for Astron
 omy and Astrophysics (IUCAA)\, India)\nEccentric compact binary coalescenc
 es (CBCs) are expected to be observed in current and future gravitational-
 wave (GW) detector networks. Such detections are especially valuable as th
 ey can provide insights on the environments that nurture CBCs. However\, i
 t has been recently pointed out that a number of other physical and beyond
 -GR effects could imitate\, or be mimicked by\, eccentric CBCs. The standa
 rd approach to ascertain that a detected CBC is eccentric is to employ Bay
 esian model selection\, where the eccentric CBC hypothesis is compared aga
 inst other hypotheses. Such an approach is not only computationally intens
 ive and time-consuming\, but could also be misleading if none of the model
 s under consideration represent the true model. In this work\, we propose 
 a conceptually simple but powerful method to directly confirm or reject th
 e eccentric hypothesis\, without needing to compare the hypothesis with th
 e plethora of other possible hypotheses. The key idea is that while spurio
 us nonzero values of eccentricity\, at some reference frequency\, could be
  acquired when a noneccentric CBC with additional physical/beyond-GR effec
 ts is recovered with an eccentric CBC waveform model\, the evolution of ec
 centricity with frequency will in general not be mimicked. We accordingly 
 formulate an eccentricity evolution consistency test (EECT). The method co
 mpares the eccentricity recovered at some low frequency value (e.g.\, 10 H
 z)\, evolved to higher frequencies assuming GR\, with eccentricities recov
 ered at those same higher frequencies. Discrepancy between the two eccentr
 icities at any reference frequency would violate EECT and indicate the pre
 sence of a mimicker. As a proof of concept\, assuming a few eccentric CBC 
 systems\, quasicircular CBCs with additional physics mimicking eccentricit
 y\, and an O4-like three-detector-network configuration\, we demonstrate t
 hat our proposed method is indeed able to reject mimickers at ≥ 68% conf
 idence\, while ensuring that truly eccentric CBCs satisfy EECT\n\nhttps://
 indico.narit.or.th/event/236/contributions/811/
LOCATION:National Astronomical Research Institute of Thailand (NARIT) Andr
 omeda Meeting Room
URL:https://indico.narit.or.th/event/236/contributions/811/
END:VEVENT
END:VCALENDAR
