Constraints on Holographic cosmologies from strong lensing systems

Abstract

We use strongly gravitationally lensed (SGL) systems to put additional constraints on a set of holographic dark energy models. Data available in the literature (redshift and velocity dispersion) is used to obtain the Einstein radius and compare it with model predictions. We found that the LCDM is the best fit to the data. Although a preliminary statistical analysis seems to indicate that two of the holographic models studied show interesting agreement with observations, a stringent test lead us to the result that neither of the holographic models are competitive with the LCDM. These results highlight the importance of Strong Lensing measurements to provide additional observational constraints to alternative cosmological models, which are necessary to shed some light into the dark universe.

21 pages, 6 figures

References in corpus (16)

• Dynamics of dark energy
• Cosmology and the Fate of Dilatation Symmetry
• Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation
• A Holographic Dark Energy Model from Ricci Scalar Curvature
• The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample
• Infrared cut-off proposal for the Holographic density
• The Structure & Dynamics of Massive Early-type Galaxies: On Homology, Isothermality and Isotropy inside one Effective Radius
• Hubble parameter measurement constraints on the cosmological deceleration-acceleration transition redshift
• Statefinder Diagnosis for Ricci Dark Energy
• Interacting holographic dark energy
• ALMA Observations of SPT-Discovered, Strongly Lensed, Dusty, Star-Forming Galaxies
• Constraints on f(R) cosmologies from strong gravitational lensing systems
• Mass models and environment of the new quadruply lensed quasar SDSS J1330+1810
• Dark Energy: A Unifying View
• A twelve-image gravitational lens system in the z ~ 0.84 cluster Cl J0152.7-1357
• Strong Gravitational Lensing and Its Cosmic Constraints

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• A magnified glance into the dark sector: probing cosmological models with strong lensing in A1689
• Holographic energy density, dark energy sound speed, and tensions in cosmological parameters: $H_0$ and $S_8$