The Nature of Gravitational Wave Events with Host Environment Escape Velocities
Guo-Peng Li, Xi-Long Fan

TL;DR
This paper introduces a new method utilizing host environment escape velocities to improve parameter estimation and origin inference of gravitational wave events, especially for hierarchical triple mergers, demonstrated on recent LIGO-Virgo-KAGRA data.
Contribution
The paper presents a novel approach using escape velocities to better constrain the properties and origins of gravitational wave sources, enhancing analysis of hierarchical mergers.
Findings
Posterior spin distributions concentrate near zero.
Uncertainty in primary mass distribution is significantly reduced.
Rules out certain events originating from globular clusters.
Abstract
We propose a novel method to probe the parameters and origin channels of gravitational wave events using the escape velocities of their host environments. This method could lead to more convergent posterior distributions offering additional insights into the physical properties, formation, and evolution of the sources. The method provides more accurate parameter estimation for events that represent previous mergers in the hierarchical triple merger scenario and is valuable for the search for such mergers with third-generation ground-based detectors. To demonstrate this approach, we take six recently identified events in LIGO-Virgo-KAGRA data, considered as potential previous mergers in hierarchical triple mergers, as examples. The use of escape velocities results in posterior spin distributions that are concentrated near zero, aligning with the expected birth spins of first-generation…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGeophysics and Gravity Measurements · Pulsars and Gravitational Waves Research · Material Science and Thermodynamics
