Reconstruction of f(G) gravity with ordinary and entropy-corrected (m,n) type Holographic dark energy model

2014/03/01 by Rahul Ghosh, Ghosh, Rahul, Ujjal Debnath +1
Earth and Planetary Sciences · Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Geophysics and Gravity Measurements #gr-qc

paper · pdf · doi:10.48550/arxiv.1403.0926

11 pages, 6 figures. arXiv admin note: text overlap with arXiv:1205.0209 by other authors

arxiv created 2014/03/01 · openalex publication_date 2014/03/01 · arxiv updated 2014/03/05 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We have discussed the correspondence of the well-accepted f(G) gravity theory with two dark energy models : (m,n)-type holographic dark energy [(m,n)-type HDE] and entropy-corrected (m,n)-type holographic dark energy. For this purpose, we have considered the power law form of the scale factor a(t)=a₀t^p, p>1. The reconstructed f(G) in these models have been found and the models in both cases are found to be realistic. We have also discussed the classical stability issues in both models. The (m,n)-type HDE and its entropy-corrected versions are more stable than the ordinary HDE model.

Citations

• (m,n)-type holographic dark energy models

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