Do we really need alternatives to the omega 0 omega a CDM parameterization after the DESI DR2?
Youri Carloni, Orlando Luongo, Marek Biesiada
astro-ph.CO, gr-qc
Submitted: 2026-08-02
Comments: 15 pages, 7 figures, 4 tables
Code: https://github.com/brinckmann/montepython_public
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Dynamical Dark Energy in light of the DESI DR2 Baryonic Acoustic Oscillations Measurements
- Quintessential interpretation of the evolving dark energy in light of DESI
- Interpreting DESI 2024 BAO: late-time dynamical dark energy or a local effect?
- Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
- Characterizing repulsive gravity with curvature eigenvalues
- Toward an invariant definition of repulsive gravity
- Dark Energy and the Accelerating Universe
- The Physics of Cosmic Acceleration
- Dark energy constraints using gamma-ray burst correlations with DESI 2024 data
- Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs
- Cosmic distance duality after DESI 2024 data release and dark energy evolution
- Testing generalized logotropic models with cosmic growth
- Unifying the dark sector through a single matter fluid with non-zero pressure
- Cosmological constraints from calibrated $E_p-E_{iso}$ gamma-ray burst correlation by using DESI 2024 data release
- Intermediate redshift calibration of Gamma-ray Bursts and cosmic constraints in non-flat cosmology
- Cosmological transition epoch from gamma-ray burst correlations
- Phase-space analysis of dark energy models in non-minimally coupled theories of gravity
- Dark Energy and Dark Matter from an additional adiabatic fluid
- Tracing dark energy history with gamma ray bursts
- Observational Probes of Cosmic Acceleration
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