Prospects for characterizing Population III remnants with next-generation gravitational-wave observatories

arXiv:2608.05846 · astro-ph.HE · Submitted 2026-08-06 · Read on arXiv

N. V. Krishnendu, Patricia Schmidt, Geraint Pratten

astro-ph.HE

Submitted: 2026-08-06

Comments: 18 pages, 12 figures in the main file and 3 figures in the appendix

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

Bayesian Inference — 11× in this paper · explained in 5 episodes
Einstein Telescope — 7× in this paper
Cosmic Explorer — 5× in this paper
Accuracy — 3× in this paper · explained in 1 episode
Bayesian Framework — 3× in this paper · explained in 3 episodes
Calibration — 2× in this paper · explained in 7 episodes
Metallicity — 2× in this paper · explained in 3 episodes
Weak Lensing — 2× in this paper · explained in 2 episodes
AGN — 1× in this paper · explained in 1 episode
Consistency — 1× in this paper · explained in 3 episodes
Gravitational Lensing — 1× in this paper · explained in 2 episodes
JWST Advanced Deep Extragalactic Survey — 1× in this paper
Non-Gaussianity — 1× in this paper · explained in 2 episodes
Population Synthesis — 1× in this paper · explained in 2 episodes
Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

Sources

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