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.
These modifications seek a deeper understanding of the universe’s nature and dynamics
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Probing Dark Energy Properties with Barrow Holographic Model in f(Q, C) Gravity
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.