Interacting dark energy constraints from Fermi GRBs and Pantheon+ SNe Ia with full GRB covariance

arXiv:2606.00549 · astro-ph.CO · Submitted 2026-05-30 · Read on arXiv

astro-ph.CO

Submitted: 2026-05-30

Updated: 2026-10-03

Comments: 29 pages, 10 figures, 4 tables; 18 pages, 7 figures; Revised version, added new experiments in Section 4

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

Terminology

Calibration — 22× in this paper · explained in 7 episodes
Amati Relation — 10× in this paper · explained in 1 episode
Hubble Tension — 5× in this paper · explained in 9 episodes
Weak Lensing — 5× in this paper · explained in 2 episodes
Adam — 4× in this paper · explained in 2 episodes
Quintessence — 4× in this paper · explained in 2 episodes
Clustering — 3× in this paper · explained in 2 episodes
Degeneracy — 3× in this paper · explained in 3 episodes
Metallicity — 3× in this paper · explained in 3 episodes
Anisotropy — 2× in this paper · explained in 3 episodes
Gravitational Lensing — 2× in this paper · explained in 2 episodes
Robustness — 2× in this paper · explained in 5 episodes
Akaike Information Criterion — 1× in this paper
Bayesian Information Criterion — 1× in this paper
Consistency — 1× in this paper · explained in 3 episodes
Gamma-ray Burst Monitor — 1× in this paper
Momentum transfer — 1× in this paper · explained in 2 episodes
Nonminimal coupling — 1× in this paper · explained in 2 episodes

Related papers