Image de couverture de livre

Cosmic distance duality after DESI 2024 data release and dark energy evolution

Fuente: arXiv

Enregistré dans:

Détails bibliographiques
Auteurs principaux:	Alfano, Anna Chiara, Luongo, Orlando
Format:	Preprint
Publié:	2025
Sujets:	Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

Documents similaires

Dark energy constraints using gamma-ray burst correlations with DESI 2024 data
par: Alfano, Anna Chiara, et autres
Publié: (2024)

Cosmological constraints from calibrated $E_p-E_{iso}$ gamma-ray burst correlation by using DESI 2024 data release
par: Alfano, Anna Chiara, et autres
Publié: (2024)

Investigating the cosmic distance duality relation with gamma-ray bursts
par: Alfano, Anna Chiara, et autres
Publié: (2025)

Does dark energy really revive using DESI 2024 data?
par: Carloni, Youri, et autres
Publié: (2024)

Breaking the baryon-dark matter degeneracy in a model-independent way through the Sunyaev-Zeldovich effect
par: Alfano, Anna Chiara, et autres
Publié: (2023)

Mapping the redshift drift at various redshifts through cosmography
par: Alfano, Anna Chiara, et autres
Publié: (2026)

Constraints on Chiral-Quintom dark energy after DESI DR2 and impact on unifying dark energy with inflation
par: Paliathanasis, Andronikos, et autres
Publié: (2025)

Model independent cosmographic constraints from DESI 2024
par: Luongo, Orlando, et autres
Publié: (2024)

Cosmological transition epoch from gamma-ray burst correlations
par: Alfano, Anna Chiara, et autres
Publié: (2024)

Challenging the $ω_0ω_a$CDM parametrization through rational expansions in view of DESI data release
par: Carloni, Youri, et autres
Publié: (2025)

Phase-space analysis in non-minimal symmetric-teleparallel dark energy
par: Carloni, Youri, et autres
Publié: (2023)

Characterizing the equivalence between dark energy and radiation using gamma-ray bursts
par: Luongo, Orlando, et autres
Publié: (2024)

Phase-space analysis of dark energy models in non-minimally coupled theories of gravity
par: Carloni, Youri, et autres
Publié: (2024)

Dynamical dark energy in the light of DESI 2024 data
par: Roy, Nandan
Publié: (2024)

Addressing the $H_0$ tension through matter with pressure and no early dark energy
par: Carloni, Youri, et autres
Publié: (2025)

Linear and nonlinear clusterings of Horndeski-inspired dark energy models with fast transition
par: Luongo, Orlando, et autres
Publié: (2023)

Dark energy reconstructions combining BAO data with galaxy clusters and intermediate redshift catalogs
par: Luongo, Orlando, et autres
Publié: (2024)

Implications of distance duality violation for the $H_0$ tension and evolving dark energy
par: Teixeira, Elsa M., et autres
Publié: (2025)

Parameterizing quasi-quintessence and quasi-phantom fields without the nearly flat potential approximation
par: Alfano, Anna Chiara, et autres
Publié: (2025)

Impact of flavor condensate dark matter on accretion disk luminosity in spherical spacetimes
par: Capolupo, Antonio, et autres
Publié: (2025)

Modified gravity realizations of quintom dark energy after DESI DR2
par: Yang, Yuhang, et autres
Publié: (2025)

Model-agnostic assessment of dark energy after DESI DR1 BAO
par: Dinda, Bikash R., et autres
Publié: (2024)

Cosmological constraints on dark energy parametrizations after DESI 2024: Persistent deviation from standard $Λ$CDM cosmology
par: Malekjani, M., et autres
Publié: (2024)

Dark energy after pre-recombination early dark energy in light of DESI DR2 and the latest ACT and SPT data
par: Wang, Hao, et autres
Publié: (2025)

Gravitational waves from two scalar fields unifying the dark sector with inflation
par: Luongo, Orlando, et autres
Publié: (2025)

Accelerating Universe without dark energy: matter creation after DESI DR2
par: Bhattacharjee, Sauvik, et autres
Publié: (2025)

Interpreting DESI's evidence for evolving dark energy
par: Cortês, Marina, et autres
Publié: (2024)

A new diagnostic for the null test of dynamical dark energy in light of DESI 2024 and other BAO data
par: Dinda, Bikash R.
Publié: (2024)

Particle production from non-minimal coupling in a symmetry breaking potential transporting vacuum energy
par: Belfiglio, Alessio, et autres
Publié: (2023)

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background
par: Dinda, Bikash R., et autres
Publié: (2025)

Interacting dark energy after DESI DR2: a challenge for $Λ$CDM paradigm?
par: Pan, Supriya, et autres
Publié: (2025)

Revisiting holographic dark energy after DESI 2024
par: Li, Tian-Nuo, et autres
Publié: (2024)

A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension
par: Carloni, Youri, et autres
Publié: (2026)

Investigating cosmic distance duality and dark energy evolution through intermediate and high-z probes
par: Alfano, Anna Chiara
Publié: (2026)

Phenomenological emergent dark energy in the light of DESI Data Release 1
par: Hernández-Almada, A., et autres
Publié: (2024)

$f(T)$ gravity after DESI Baryon Acoustic Oscillation and DES Supernovae 2024 data
par: Escamilla-Rivera, Celia, et autres
Publié: (2024)

Evidence for dynamical dark energy from DESI-DR2 and SN data? A symbolic regression analysis
par: Sousa-Neto, Agripino, et autres
Publié: (2025)

Cosmic curvature on large-scale structures with homogeneous dark energy
par: Dinda, Bikash R.
Publié: (2023)

Geometric multipartite entanglement from gravitational particle production
par: Belfiglio, Alessio, et autres
Publié: (2025)

Comparing Bondi and Novikov-Thorne accretion disk luminosity around regular black holes
par: Capozziello, Salvatore, et autres
Publié: (2025)