Line-of-sight Acceleration Driven Effects in Eccentric Compact Binary Coalescences
gr-qc, astro-ph.HE
Submitted: 2026-10-06
Updated: 2026-10-06
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Sources
- Advanced LIGO
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- Overview of KAGRA: Detector design and construction history
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog
- GWTC-4.0: Methods for Identifying and Characterizing Gravitational-wave Transients
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-5.0: An Introduction to Version 5.0 of the Gravitational-Wave Transient Catalog
- GWTC-5.0: Methods for Identifying and Characterizing Gravitational-wave Transients
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- Measuring eccentricity in binary black hole inspirals with gravitational waves
- Constraining the orbital eccentricity of inspiralling compact binary systems with Advanced LIGO
- Gravitational Wave Detector Sensitivity to Eccentric Black Hole Mergers
- Systematic parameter errors in inspiraling neutron star binaries
- A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
- Residual eccentricity of inspiralling orbits at the gravitational-wave detection threshold: Accurate estimates using post-Newtonian theory
- Eccentric Black Hole Mergers Forming in Globular Clusters
- Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries
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