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Holographic dark matter and dark energy with second order invariants

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arxiv 1109.3177 v2 pith:KGNGAGP4 submitted 2011-09-14 gr-qc

classification gr-qc
keywords darkmatteruniversecosmicenergyholographicinvariantsmodels
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One of the main goals of modern cosmology remains to summon up a self consistent policy, able to explain, in the framework of the Einstein's theory, the cosmic speed up and the presence of Dark Matter in the Universe. Accordingly to the Holographic principle, which postulates the existence of a minimal size of a physical region, we argue, in this paper, that if this size exists for the Universe and it is accrued from the independent geometrical second order invariants, it would be possible to ensure a surprising source for Dark Matter and a viable candidate for explaining the late acceleration of the Universe. Along the work, we develop low redshift tests, such as Supernovae Ia and kinematical analysis complied by the use of Cosmography and we compare the outcomes with higher redshift tests, such as CMB peak and anisotropy of the cosmic power spectrum. All the results indicate that the models presented here can be interpreted as unified models that are capable to describe both the dark matter and the dark energy.

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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. 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.

  2. Consequences of non-minimal coupling for mass mixing in spontaneous baryogenesis

    gr-qc 2025-05 conditional novelty 5.0 of 10

    A non-minimal coupling between the inflaton and spacetime curvature is shown to enhance spontaneous baryogenesis by increasing the effective inflaton mass, yielding a new correction to the baryon asymmetry formula.

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