Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
Soumen Roy, Rodrigo Vicente

TL;DR
This study demonstrates that compact binary coalescences in dense gaseous environments can produce gravitational-wave signals indistinguishable from vacuum events in detection but cause biases in parameter estimation, highlighting the need for environmental waveform models.
Contribution
The paper introduces numerical relativity simulations showing that dense gaseous environments can mimic vacuum signals and affect parameter estimation, emphasizing the importance of environmental waveform models.
Findings
Vacuum-like detection of events in dense environments
Environmental effects cause biases in parameter estimation
Phenomenological waveforms can detect and resolve environmental effects
Abstract
The gravitational-wave events observed by the LIGO-Virgo-KAGRA collaboration are attributed to compact binary coalescences happening in vacuum. However, several studies suggest that gaseous environments may play a significant role in the formation and evolution of compact binaries. Why have we not seen environmental effects in LVK signals? While matched-filtering remains the most effective technique for gravitational-wave searches, it comes with a burden: we might only observe signals that align with our (vacuum) expectations, potentially missing unexpected or unknown phenomena. Even more concerning is the possibility that environmental effects could mimic vacuum waveforms, introducing biases in parameter estimation and impacting population studies. Here, we use numerical relativity simulations of binary black hole mergers inside stellar envelopes to show that: (i) a…
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Taxonomy
TopicsCold Atom Physics and Bose-Einstein Condensates · Quantum Mechanics and Applications
