Imagen de Portada

The Excess of JWST Bright Galaxies: a Possible Origin in the Ground State of Dynamical Dark Energy in the light of DESI 2024 Data

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autores principales:	Menci, Nicola, Sen, Anjan Ananda, Castellano, Marco
Formato:	Preprint
Publicado:	2024
Materias:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Negative cosmological constant in the dark energy sector: tests from JWST photometric and spectroscopic observations of high-redshift galaxies
por: Menci, Nicola, et al.
Publicado: (2024)

Dark energy in light of the early JWST observations: case for a negative cosmological constant?
por: Adil, Shahnawaz A., et al.
Publicado: (2023)

Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
por: Ruchika, et al.
Publicado: (2020)

Braneworld Dark Energy in light of DESI DR2
por: Mishra, Swagat S., et al.
Publicado: (2025)

UV-complete and stable Quintom Dark Energy models in the light of DESI DR2
por: Koutroulis, Fotis
Publicado: (2026)

Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?
por: Bird, Simeon, et al.
Publicado: (2023)

Quintessential Implications of the presence of AdS in the Dark Energy sector
por: Mukherjee, Purba, et al.
Publicado: (2025)

Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide
por: Antusch, Stefan, et al.
Publicado: (2026)

Dark Sector Electroweak Baryogenesis In Light Of The Galactic Center Excess
por: Roux, Jean-Samuel, et al.
Publicado: (2025)

Reduced Hubble Tension in Dark Radiation Models after DESI 2024
por: Allali, Itamar J., et al.
Publicado: (2024)

Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess
por: Hu, Yongao, et al.
Publicado: (2025)

On the Analysis Dependence of DESI Dynamical Dark Energy
por: Colgáin, Eoin Ó, et al.
Publicado: (2025)

Gravitational atoms in the braneworld scenario
por: Bohra, Sunil Singh, et al.
Publicado: (2023)

Robust Preference for Dynamical Dark Energy in DESI BAO and SN Measurements
por: Giarè, William, et al.
Publicado: (2024)

Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements
por: Giarè, William, et al.
Publicado: (2024)

How Theory-Informed Priors Affect DESI Evidence for Evolving Dark Energy
por: Toomey, Michael W., et al.
Publicado: (2025)

Exotic Dark Matter and the DESI Anomaly
por: Braglia, Matteo, et al.
Publicado: (2025)

Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots
por: Feng, Wei-Xiang, et al.
Publicado: (2025)

Implications of DESI for Dark Matter & Cosmic Birefringence
por: Barman, Basabendu, et al.
Publicado: (2025)

The Self-Consistency of DESI Analysis and Comment on "Does DESI 2024 Confirm $Λ$CDM?"
por: Wang, Deng
Publicado: (2024)

Quintessence and phantoms in light of DESI 2025
por: Gialamas, Ioannis D., et al.
Publicado: (2025)

Multi-Component Dark Matter as a Solution to the Galactic Center GeV Excess
por: Queiroz, Farinaldo S., et al.
Publicado: (2026)

Spherical Collapse Approach for Non-standard Dark Matter Models and Enhanced Early Galaxy Formation in JWST
por: Davari, Zahra, et al.
Publicado: (2023)

Impact of ACT DR6 and DESI DR2 for Early Dark Energy and the Hubble tension
por: Poulin, Vivian, et al.
Publicado: (2025)

Bounce Inflation with Dynamical Dark Energy in Light of DESI DR2
por: Zhang, Xin-zhe, et al.
Publicado: (2026)

Neutrinos with refractive masses and the DESI BAO results
por: Sen, Manibrata, et al.
Publicado: (2024)

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses
por: Chudaykin, Anton, et al.
Publicado: (2025)

Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST
por: Das, Souradeep, et al.
Publicado: (2025)

Probing the Evolution of Dark Energy: A Joint Analysis of DESI DR2, Pantheon+, and Cosmic Chronometers
por: Kumari, Chanchal, et al.
Publicado: (2026)

From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
por: Bottaro, Salvatore, et al.
Publicado: (2024)

Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO
por: Granelli, Alessandro, et al.
Publicado: (2026)

UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings
por: Blamart, Mattéo, et al.
Publicado: (2025)

Cosmological Constraints on the Phenomenological Interacting Dark Energy Model with Fermi Gamma-Ray Bursts and DESI DR2
por: Zhu, Ziyan, et al.
Publicado: (2025)

Thermodynamic Origin of the Tully-Fisher Relation in Dark Matter Dominated Galaxies: A Theoretical-Empirical Derivation
por: Oikonomou, V. K.
Publicado: (2025)

Thawing quintessence and transient cosmic acceleration in light of DESI
por: de Souza, Rayff, et al.
Publicado: (2025)

Simple quintessence models in light of DESI-BAO observations
por: Cline, James M., et al.
Publicado: (2025)

Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess
por: Nomura, Yasunori, et al.
Publicado: (2026)

Supernova-Neutrino-Boosted Dark Matter from All Galaxies
por: Lin, Yen-Hsun, et al.
Publicado: (2024)

Dark Acoustic Oscillations as an Early-Universe Explanation of the DESI Anomaly
por: Garny, Mathias, et al.
Publicado: (2025)

Fitting the DESI BAO Data with Dark Energy Driven by the Cohen-Kaplan-Nelson Bound
por: Adolf, Patrick, et al.
Publicado: (2024)