Cosmological constraints and standard sirens forecasts for non-dynamical dark energy in Horndeski gravity

arXiv:2608.04079 · astro-ph.CO, gr-qc · Submitted 2026-08-04 · Read on arXiv

Marcello Miranda, Ruchika, Ivan De Martino, Daniele Vernieri, Salvatore Capozziello

astro-ph.CO, gr-qc

Submitted: 2026-08-04

Comments: 23 pages, 19 figures, 2 tables

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

Terminology

Benchmark — 11× in this paper · explained in 2 episodes
Calibration — 9× in this paper · explained in 7 episodes
Lunar Laser Ranging — 7× in this paper
Big Bang Nucleosynthesis — 5× in this paper
Consistency — 4× in this paper · explained in 3 episodes
Cosmic Explorer — 4× in this paper
Einstein Telescope — 4× in this paper
Bayesian Inference — 3× in this paper · explained in 5 episodes
Trace — 2× in this paper · explained in 2 episodes
Abundance — 1× in this paper · explained in 1 episode
Alignment — 1× in this paper · explained in 1 episode
Aperture — 1× in this paper · explained in 1 episode
Baryon Acoustic Oscillations — 1× in this paper
Cooperation — 1× in this paper · explained in 2 episodes
Core — 1× in this paper · explained in 2 episodes
Fisher Information — 1× in this paper · explained in 3 episodes
Fisher Information Matrix — 1× in this paper
Hubble Tension — 1× in this paper · explained in 9 episodes
Normalizing Flow — 1× in this paper · explained in 3 episodes
Normalizing Flows — 1× in this paper · explained in 4 episodes
Population Synthesis — 1× in this paper · explained in 2 episodes
Signal-to-Noise Ratio — 1× in this paper
Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes
Soft X-ray Imager — 1× in this paper

Sources

Related papers