A Critique of Holographic Dark Energy
Eoin \'O Colg\'ain, M. M. Sheikh-Jabbari

TL;DR
This paper critically examines holographic dark energy models, highlighting observational constraints, theoretical inconsistencies such as NEC violation, and comparing their fit to data with the standard flat Lambda Cold Dark Matter model.
Contribution
It provides a detailed critique of HDE, demonstrating observational and theoretical issues, and compares its performance against the flat Lambda CDM model.
Findings
HDE predicts a future turning point in H(z) incompatible with observations.
Turning points in HDE violate the Null Energy Condition.
Flat Lambda CDM fits data better than HDE.
Abstract
Observations restrict the parameter space of Holographic Dark Energy (HDE) so that a turning point in the Hubble parameter is inevitable. Concretely, cosmic microwave background (CMB), baryon acoustic oscillations (BAO) and Type Ia supernovae (SNE) data put the turning point in the future, but removing SNE results in an observational turning point at positive redshift. From the perspective of theory, not only does the turning point violate the Null Energy Condition (NEC), but as we argue, it may be interpreted as an evolution of the Hubble constant with redshift, which is at odds with the very FLRW framework within which data has been analysed. Tellingly, neither of these are problems for the flat CDM model, and a direct comparison of fits further disfavours HDE relative to flat CDM.
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