Imagen de Portada

Can acoustic and axion-like early dark energy still resolve the Hubble tension?

Fuente: arXiv

Guardado en:

Detalles Bibliográficos
Autor principal:	Simon, Théo
Formato:	Preprint
Publicado:	2023
Materias:	Cosmology and Nongalactic Astrophysics
Acceso en línea:	Acceder al recurso
Etiquetas:	Agregar Etiqueta Sin Etiquetas, Sea el primero en etiquetar este registro!

Ejemplares similares

Can interacting dark energy with dynamical coupling resolve the Hubble tension
por: Yao, Yan-Hong, et al.
Publicado: (2022)

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension
por: Bella, Marco, et al.
Publicado: (2026)

Role of dynamical early dark energy in Hubble tension through warm inflation
por: B, Anupama
Publicado: (2025)

A convenient approach to characterizing model uncertainty with application to early dark energy solutions of the Hubble tension
por: Paradiso, S., et al.
Publicado: (2023)

Restoring cosmological concordance with axion-like early dark energy and dark matter characterized by a constant equation of state?
por: Yao, Yan-Hong, et al.
Publicado: (2023)

Omnipotent dark energy: A phenomenological answer to the Hubble tension
por: Adil, Shahnawaz A., et al.
Publicado: (2023)

Constraints on interacting dark energy revisited: implications for the Hubble tension
por: Hoerning, Gabriel A., et al.
Publicado: (2023)

On the interacting dark energy scenarios $-$ the case for Hubble constant tension
por: Pan, Supriya, et al.
Publicado: (2023)

Revisiting the Hubble tension problem in the framework of holographic dark energy
por: Li, Jun-Xian, et al.
Publicado: (2025)

Hubble tension may indicate time-dependent dark matter comoving energy density
por: Kitazawa, Noriaki
Publicado: (2024)

Disentangling cosmic distance tensions with early and late dark energy
por: Jhaveri, Tanisha, et al.
Publicado: (2026)

Hubble tension as a window on the gravitation of the dark matter sector
por: Pitrou, Cyril, et al.
Publicado: (2023)

Oscillating dark energy in light of the latest observations and its impact on the Hubble tension
por: Rezaei, Mehdi
Publicado: (2024)

What solves the Hubble tension in phenomenological dark energy models at background level?
por: Manoharan, Manosh T.
Publicado: (2025)

Multi-axion like description of the dark sector in light of the Hubble and $σ_8$ tensions
por: Dumancic, John, et al.
Publicado: (2025)

Can cosmic rotation resolve the Hubble tension? Constraints from CMB and large-scale structure
por: Benetti, Micol, et al.
Publicado: (2025)

Accelerated inference on accelerated cosmic expansion: New constraints on axion-like early dark energy with DESI BAO and ACT DR6 CMB lensing
por: Qu, Frank J., et al.
Publicado: (2024)

DESI constraints on the varying electron mass model and axion-like early dark energy
por: Seto, Osamu, et al.
Publicado: (2024)

Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
por: Montani, Giovanni, et al.
Publicado: (2025)

A solution to the Hubble tension with self-interacting ultralight dark matter
por: Lee, Jae-Weon
Publicado: (2025)

Updated cosmological constraints on axion dark energy with DESI
por: Ureña-López, L. A., et al.
Publicado: (2025)

Beyond LambdaCDM: How the Hubble tension challenges early universe physics
por: Simpson, Gawain, et al.
Publicado: (2025)

Toward a simultaneous resolution of the $H_0$ and $S_8$ tensions: early dark energy and an interacting dark sector model
por: Yashiki, Mai
Publicado: (2025)

Cosmological constraints on early dark energy from the full shape analysis of eBOSS DR16
por: Gsponer, Rafaela, et al.
Publicado: (2023)

Cosmic acceleration and the Hubble tension from baryon acoustic oscillation data
por: Lu, Xuchen, et al.
Publicado: (2024)

Modified recombination and the Hubble tension
por: Mirpoorian, Seyed Hamidreza, et al.
Publicado: (2024)

Hubble tension as a window on the gravitation of the dark matter sector: Exploration of a family of models
por: Uzan, Jean-Philippe, et al.
Publicado: (2023)

Can dynamic dark energy explain the $S_8$ tension, the `lensing is low' effect, or strong baryon feedback?
por: Heydenreich, S., et al.
Publicado: (2025)

A flexible parameterization to test early physics solutions to the Hubble tension with future CMB data
por: Kou, Raphaël, et al.
Publicado: (2024)

Addressing the $H_0$ tension through matter with pressure and no early dark energy
por: Carloni, Youri, et al.
Publicado: (2025)

Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters
por: Aboubrahim, Amin, et al.
Publicado: (2025)

High-redshift, small-scale tests of ultralight axion dark matter using Hubble and Webb galaxy UV luminosities
por: Winch, Harrison, et al.
Publicado: (2024)

Decay of dark energy into dark matter in a metric $f(R)$ gravity: effective running Hubble constant
por: Montani, Giovanni, et al.
Publicado: (2025)

Dark energy in light of recent DESI BAO and Hubble tension
por: Wang, Hao, et al.
Publicado: (2024)

The effective running Hubble constant in SNe Ia as a marker for the dark energy nature
por: Fazzari, E., et al.
Publicado: (2025)

Cuscuton-like contribution to dark energy evolution
por: Bazeia, D., et al.
Publicado: (2025)

DESI and the Hubble tension in light of modified recombination
por: Lynch, Gabriel P., et al.
Publicado: (2024)

On the impact of the supernova subsamples in reducing the Hubble tension
por: Martins, Gonçalo, et al.
Publicado: (2025)

New multiprobe analysis of modified gravity and evolving dark energy
por: Lu, Zhiyu, et al.
Publicado: (2025)

Results from Hubble parameter data: oscillating dark energy?
por: Yang, Rong-Jia
Publicado: (2025)