Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook
Tristan S. Weaver, David Radice, Donghui Jeong, Victor Liu
The Pennsylvania State University · The Pennsylvania State University · Korea Institute for Advanced Study · The Pennsylvania State University
astro-ph.HE, astro-ph.SR, gr-qc
Submitted: 2026-07-27
Comments: 19 pages, 9 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Observation of Gravitational Waves from a Binary Black Hole Merger
- Advanced LIGO
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- GstLAL O4 Online Results Paper
- GWTC-5.0: Observations from the Second Part of the Fourth LIGO-Virgo-KAGRA Observing Run and Updates to the Gravitational-Wave Transient Catalog
- GWTC-5.0: Population Properties of Merging Compact Binaries
- Population properties and multimessenger prospects of neutron star-black hole mergers following GWTC-3
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
- Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
- Rates of Compact Object Coalescences
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Advanced Virgo: a 2nd generation interferometric gravitational wave detector
- KAGRA: 2.5 Generation Interferometric Gravitational Wave Detector
- Cosmic Explorer: A Submission to the NSF MPSAC ngGW Subcommittee
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- The North American Nanohertz Observatory for Gravitational Waves
- The International Pulsar Timing Array
- The International Pulsar Timing Array: Second data release
- Laser Interferometer Space Antenna
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