Cosmological Constraints from Gravitational Wave-Fast Radio Burst Associations without Redshift Measurements for LIGO-Virgo and Cosmic Explorer
astro-ph.CO, astro-ph.HE
Submitted: 2026-04-03
Updated: 2026-09-10
Code: https://github.com/MariosNT/FRB
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- GW190521 as a black-hole merger coincident with the ZTF19abanrhr flare
- NE2001.I. A New Model for the Galactic Distribution of Free Electrons and its Fluctuations
- NE2001. II. Using Radio Propagation Data to Construct a Model for the Galactic Distribution of Free Electrons
- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
- A Horizon Study for Cosmic Explorer: Science, Observatories, and Community
- The DSA-2000 -- A Radio Survey Camera
- Hubble Constant Measurement with GW190521 as an Eccentric Black Hole Merger
- Cosmology with Fast Radio Bursts
- Breaking the Baryon Density$\unicode{x2013}$Hubble Constant Degeneracy in Fast Radio Burst Applications with Associated Gravitational Waves
- Ray-tracing Fast Radio Bursts Through IllustrisTNG: Cosmological Dispersion Measures from Redshift 0 to 5.5
- Multilevel and hierarchical Bayesian modeling of cosmic populations
- Beyond Gaps and Bumps: Spectral Siren Cosmology with Non-Parametric Population Models
- First measurement of the Hubble parameter from bright binary black hole GW190521
- Gravitational Wave Cosmology
- Estimating Hubble Constant with Gravitational Observations: A Concise Review
- A unified harmonic framework for dark siren cosmology
- A Comprehensive Measurement of the Local Value of the Hubble Constant with 1 km/s/Mpc Uncertainty from the Hubble Space Telescope and the SH0ES Team
- GWTC-4.0: Updating the Gravitational-Wave Transient Catalog with Observations from the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run
- GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation
- GWTC-4.0: Population Properties of Merging Compact Binaries
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