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Entropic corrections and modified Friedmann equations in the emergence of cosmic space

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arxiv 1304.7949 v3 pith:DNDRVMAC submitted 2013-04-30 gr-qc

Entropic corrections and modified Friedmann equations in the emergence of cosmic space

classification gr-qc
keywords correctionscosmicentropicequationsexpansionfriedmannmodifiedspace
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In the emergent cosmic space scenario recently proposed by Padmanabhan, the expansion of the universe is attributed to the difference between the number of degrees of freedom on a holographic surface and the one in the bulk. Based on this idea, we explore the cases where logarithmic and power-law entropic corrections are present, respectively. The previously found modified Friedmann equations are reproduced through an improved proposal, and we show that the same results can be obtained using a generalized expansion law.

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Cited by 1 Pith paper

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  1. Observational Constraints on Emergent Fractional Fractal Cosmology

    gr-qc 2026-07 conditional novelty 4.0

    Joint SN+H(z)+fσ8+BAO+CMB analysis constrains the EFF fractal dimension to d=2.0004^{+0.0006}_{-0.0003}, with BIC favoring plain ΛCDM.