Phase Space of Binary Black Holes from Gravitational Wave Observations to Unveil its Formation History
Samsuzzaman Afroz, Suvodip Mukherjee

TL;DR
This paper introduces the BCO Phase Space concept to connect gravitational wave observations with binary black hole formation models, providing new insights into their origins and evolution over cosmic time.
Contribution
It presents a novel BCO Phase Space framework that links GW data to formation channels, applied to GWTC-3, revealing potential primordial origins for some events.
Findings
GW190425 and GW230529 may originate from primordial black hole growth scenarios.
BCO Phase Space can differentiate formation channels with more GW data.
The approach offers new insights into BCO evolution across cosmic history.
Abstract
Gravitational Wave (GW) sources offer a valuable window to the physical processes that govern the formation of binary compact objects (BCOs). However, deciphering such information from GW data is substantially challenging due to the difficulty in mapping from the space of observation to the space of numerous theoretical models. We introduce the concept of BCO Phase-Space that connects the observable space to the evolution trajectories of the BCO formation channels with cosmic time and apply it to the third GW transient catalog (GWTC-3) that brings new insights into probable astrophysical formation scenarios of nearly events. Our study reveals that two events, GW190425 and GW230529, show an overlap with a \texttt{BCO Phase Space} trajectory of the same formation channel arising from a sub-solar mass black hole scenario that has grown into a higher mass by accretion, hinting towards…
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Taxonomy
TopicsRelativity and Gravitational Theory · Cosmology and Gravitation Theories · Pulsars and Gravitational Waves Research
