Line-of-Sight Acceleration-driven waveform corrections for unequal-mass 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
- 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
- Searching for Eccentricity: Signatures of Dynamical Formation in the First Gravitational-Wave Transient Catalogue of LIGO and Virgo
- AGN as Potential Factories for Eccentric Black Hole Mergers
- Implications of Eccentric Observations on Binary Black Hole Formation Channels
- Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
- Merging stellar-mass binary black holes
- The First Two Years of Electromagnetic Follow-Up with Advanced LIGO and Virgo
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