Parameter Estimation for Low-Mass Eccentric Black Hole Binaries

Understand

Recent studies have shown that orbital eccentricity may indicate dynamical assembly as a formation mechanism for binary black holes.

• Eccentricity leaves a distinct signature in gravitational wave signals and it may be measured if the binary remains eccentric when it enters the LIGO band.
• Although eccentricity has not yet been confidently detected, the possibility of detecting eccentric binaries is becoming more likely with the improved sensitivity of gravitational wave detectors such as LIGO, Virgo, and KAGRA.
• It is crucial to assess the accuracy of current search pipelines in recovering eccentricity from gravitational wave signals if it is present.