Cover Image

What solves the Hubble tension in phenomenological dark energy models at background level?

Fuente: arXiv

Saved in:

Bibliographic Details
Main Author:	Manoharan, Manosh T.
Format:	Preprint
Published:	2025
Subjects:	Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Similar Items

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

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

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

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

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

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

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

2D BAO vs 3D BAO: solving the Hubble tension with an alternative cosmological model
by: Dwivedi, Sowmaydeep, et al.
Published: (2024)

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

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

A parameterized equation of state for dark energy and Hubble Tension
by: Zhao, Jing-Ya, et al.
Published: (2025)

Parametrizing the Hubble function instead of dark energy: Many possibilities
by: Paul, Sivasish, et al.
Published: (2025)

A new parametrization of Hubble function and Hubble tension
by: He, Tong-Yu, et al.
Published: (2024)

Barrow Interacting holographic dark energy cosmology with Hubble horizon as IR cutoff: A model can Alleviating the Hubble and $S_{8}$ Tension
by: Yarahmadi, Muhammad
Published: (2025)

Effective chemical potential and its phenomenological implications for the Hubble parameter
by: Sales, L. L., et al.
Published: (2026)

Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
by: Dai, Xinyi, et al.
Published: (2026)

Addressing the Hubble tension in Yukawa cosmology?
by: Jusufi, Kimet, et al.
Published: (2024)

A null test of the Hubble tension
by: Kouniatalis, Gerasimos, et al.
Published: (2026)

Interaction in the dark sector: a phenomenological approach
by: Santana, Z. C., et al.
Published: (2024)

The Hubble parameter of the Local Distance Ladder from dynamical dark energy with no free parameters
by: van Putten, Maurice H. P. M.
Published: (2024)

Multiple transitions in vacuum dark energy and $H_0$ tension
by: Moshafi, Hossein, et al.
Published: (2022)

The Hubble tension from the standpoint of quantum cosmology
by: Kuzmichev, V. E., et al.
Published: (2022)

Slow-rolling scalar dynamics and as solution for the Hubble tension
by: Montani, Giovanni, et al.
Published: (2023)

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

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

Interacting dark energy models
by: Rugg, Robert, et al.
Published: (2024)

A possible solution to the Hubble tension from quantum gravity
by: B, Anupama, et al.
Published: (2023)

Scaling solutions as Early Dark Energy resolutions to the Hubble tension
by: Copeland, Edmund J., et al.
Published: (2023)

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background
by: Dinda, Bikash R., et al.
Published: (2025)

A gravitational constant transition within cepheids as supernovae calibrators can solve the Hubble tension
by: Ruchika, et al.
Published: (2023)

Running gravitational constant induced dark energy as a solution to $σ_8$ tension
by: Zhumabek, Tilek, et al.
Published: (2024)

Cluster number counts in dark energy model with energy and momentum coupling to dark matter
by: Wongsangwal, Chattree, et al.
Published: (2026)

Bimetric gravity improves the fit to DESI BAO and eases the Hubble tension
by: Högås, Marcus, et al.
Published: (2025)

Cosmic voids and the kinetic analysis. IV. Hubble tension and the cosmological constant
by: Gurzadyan, V. G., et al.
Published: (2025)

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

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

Cosmic acceleration driven by dark matter self-interactions: a phenomenological treatment
by: Çamlıbel, A. Kazım
Published: (2019)

Lensing amplitude anomaly and varying electron mass alleviate the Hubble and $S_8$ tensions
by: Wang, Yi-Ying, et al.
Published: (2025)

Thermodynamics of sign-switching dark energy models
by: Tamayo, David
Published: (2025)

Cosmic voids and the kinetic analysis. V. Hubble tension, the cosmological constant and aperiodic filaments
by: Gurzadyan, V. G., et al.
Published: (2025)