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Holographic Dark Energy from Fluid/Gravity Duality Constraint by Cosmological Observations

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arxiv 1704.03281 v4 pith:NNLJ7YLK submitted 2017-04-06 hep-th gr-qc

Behnam Pourhassan , Alexander Bonilla , Mir Faizal , Everton M. C. Abreu This is my paper · ORCID
classification hep-thgr-qc
keywords modeldualityfluidgravitycosmologicaldarkenergyholographic
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In this paper, we obtain a holographic model of dark energy using the fluid/gravity duality. This model will be dual to a higher dimensional Schwarzschild black hole, and we would use fluid/gravity duality to relate to the parameters of this black hole to such a cosmological model. We will also analyze the thermodynamics of such a solution, and discuss the stability model. Finally, we use cosmological data to constraint the parametric space of this dark energy model. Thus, we will use observational data to perform cosmography for this holographic model based on fluid/gravity duality.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Holographic bounce

    gr-qc 2019-08 conditional novelty 6.0 of 10

    Holographic infrared and ultraviolet cutoffs can produce bouncing solutions, including nonsingular ones, and can be designed to reproduce F(R) gravity bounce.

  2. Constraints on Barrow and Tsallis Holographic Dark Energy from DESI DR2 BAO data

    gr-qc 2025-06 conditional novelty 5.0 of 10

    Barrow and Tsallis holographic dark energy models fit DESI DR2 data but are disfavored by information criteria versus LambdaCDM and do not ease the Hubble tension.

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