Results 101 to 110 of about 1,833,333 (166)

Gaussian Process Approach for Model-independent Reconstruction of f(Q) Gravity with Direct Hubble Measurements

open access: yesThe Astrophysical Journal
The increase of discrepancy in the standard procedure to choose the arbitrary functional form of the Lagrangian f ( Q ) motivates us to solve this issue in modified theories of gravity. In this regard, we investigate the Gaussian process, which allows us
Gaurav N. Gadbail   +2 more
doaj   +1 more source

Impact of Teleparallelism on Addressing Current Tensions and Exploring the GW Cosmology

open access: yesThe Astrophysical Journal
The H _0 and S _8 tensions highlight critical discrepancies in modern cosmology, challenging the standard Lambda cold dark matter model. The H _0 tension arises from conflicting measurements between local probes and early-Universe predictions. Similarly,
Sai Swagat Mishra   +3 more
doaj   +1 more source

Constraining Extended Teleparallel Gravity via Cosmography: A Model-independent Approach

open access: yesThe Astrophysical Journal
As a classical approach, the dynamics of the Universe, influenced by its dark components, are unveiled through prior modifications of Einstein’s equations.
Sai Swagat Mishra   +3 more
doaj   +1 more source

Aether, dark energy and string compactifications. [PDF]

open access: yesPhilos Trans A Math Phys Eng Sci, 2022
Townsend PK.
europepmc   +1 more source

Barrow holographic dark energy with Granda-Oliveros cutoff. [PDF]

open access: yesEur Phys J Plus, 2022
Oliveros A, Sabogal MA, Acero MA.
europepmc   +1 more source

Dark Cosmology and Its Origins

open access: yesZygon
This article reviews the standard model of cosmology: an expanding universe whose expansion is now accelerating, driven by dark energy (equivalent in practice to endowing the vacuum with a constant uniform energy density).
John A. Peacock
doaj   +2 more sources

Trapped early dark energy

open access: yesPhysics Letters B
As a prospective resolution of the Hubble tension, early dark energy (EDE) suffers from the coincidence problem, why EDE is active just at matter-radiation equality (equivalently why the slope of EDE potential is required to approximately equal to the ...
Hao Wang, Yun-Song Piao
doaj   +1 more source

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