It affects how the universe ex- pands, how matter clusters, and how galaxies form

Energy density As, the energy density is essential to understanding the universe’s evolution

1 Pith paper cite this work. Polarity classification is still indexing.

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gr-qc · 2024-11-28 · reject · novelty 2.0

Assumes the Lambda-CDM expansion history, labels it Barrow holographic dark energy in f(Q,C) gravity, and fits H0 and Omega0m to standard datasets.

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Probing Dark Energy Properties with Barrow Holographic Model in f(Q, C) Gravity gr-qc · 2024-11-28 · reject · none · ref 3
Assumes the Lambda-CDM expansion history, labels it Barrow holographic dark energy in f(Q,C) gravity, and fits H0 and Omega0m to standard datasets.