Modified IDE model with interaction parameter alpha ~0.01 from late-universe data shows H0 decreasing with redshift, tightening to 10^-5 when CMB priors are added.
Paliathanasis, Observational Constraints on Scalar Field–Matter Interaction in Weyl Inte- grable Spacetime, (2025), arXiv:2506.16223 [gr-qc]
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.CO 3verdicts
UNVERDICTED 3roles
background 1polarities
background 1representative citing papers
Quintessence models with standard potentials give only modest improvements over Lambda to DESI data on evolving dark energy, while non-minimal couplings allow temporary phantom behavior but face tight gravity constraints except for carefully selected narrow ranges.
A review summarizing advancements over the past two years that link DESI baryon acoustic oscillation data to string-inspired scenarios with dynamic dark energy.
citing papers explorer
No citing papers match the current filters.