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October 12, 2025Open Access

Lovelock type brane cosmology

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The model suggests Lovelock-type brane models may explain cosmic acceleration in a five-dimensional framework.
Key findings show that at low energies, correction terms significantly influence cosmological processes and dynamics.
Using a Friedmann-Robertson-Walker geometry, the model yields a new Friedmann-type equation based on energy density parameters.
The brane expansion behavior transitions between self-accelerating and non-self-accelerating, depending on dimensional contributions.

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This analysis examines the brane gravity model's effects on cosmic acceleration and energy density parameters.

Arroyo et al. (2025) studied this question.

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