A dark-meson field from a hidden SU(3) force is presented as a parameter-free dark energy model, but the key parameter is actually fitted and the claimed fit improvement is inflated by an arithmetic error.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.CO 1years
2025 1verdicts
REJECT 1representative citing papers
citing papers explorer
-
Bound dark energy: Particle origin of dark energy with DESI BAO and DES supernova data
A dark-meson field from a hidden SU(3) force is presented as a parameter-free dark energy model, but the key parameter is actually fitted and the claimed fit improvement is inflated by an arithmetic error.