Strong lensing systems and galaxy cluster observations as probe to the cosmic distance duality relation

@article{Holanda2021StrongLS,
  title={Strong lensing systems and galaxy cluster observations as probe to the cosmic distance duality relation},
  author={Rodrigo F.L. Holanda and F. S. Lima and Akshay Rana and Deepak Jain},
  journal={The European Physical Journal C},
  year={2021},
  volume={82}
}
In this paper, we use large scale structure observations to test the redshift dependence of cosmic distance duality relation (CDDR), DL(1+z)-2/DA=η(z)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$D_\mathrm{L}(1+z)^{-2}/D_\mathrm{A}=\eta (z)$$\end{document}, with DL\documentclass[12pt]{minimal} \usepackage{amsmath… 
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References

SHOWING 1-10 OF 58 REFERENCES

Cosmography using strong-lensing systems and cosmic chronometers

Using a new sub-sample of observed strong gravitational lens systems, for the first time, we present the equation for the angular diameter distance in the y-redshift scenario for cosmography and

Testing the distance-duality relation with the baryon acoustic oscillations data and type Ia supernovae data

  • Jun Chen
  • Physics
    Communications in Theoretical Physics
  • 2020
In this letter, the cosmic distance-duality relation has been constrained with a model-independent method by combining the baryon acoustic oscillation (BAO) data and the type Ia supernova (SNe Ia)

Determining Model-independent H0 and Consistency Tests

We determine the Hubble constant H0 precisely (2.3% uncertainty) in a manner independent of the cosmological model through Gaussian process regression, using strong lensing and supernova data. Strong

Multiple Measurements of Quasars Acting as Standard Probes: Exploring the Cosmic Distance Duality Relation at Higher Redshift

General relativity reproduces main current cosmological observations, assuming the validity of the cosmic distance duality relation (CDDR) at all scales and epochs. However, CDDR is poorly tested in

A Model-independent Determination of the Hubble Constant from Lensed Quasars and Supernovae Using Gaussian Process Regression

Strongly lensed quasar systems with time delay measurements provide “time delay distances,” which are a combination of three angular diameter distances and serve as powerful tools to determine the

H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes

We present a measurement of the Hubble constant (H0) and other cosmological parameters from a joint analysis of six gravitationally lensed quasars with measured time delays. All lenses except the

Testing dark energy models with a new sample of strong-lensing systems

Inspired by a new compilation of strong lensing systems, which consist of 204 points in the redshift range $0.0625 1$ or high velocity dispersion $\sigma > 276$ km s$^{-1}$). However, we obtained a

Setting limits on q0 from gravitational lensing

Gravitational lensing by galaxies in a wide variety of cosmological models is considered. For closed models, the lensing depends on the parameter beta(crit). If beta(crit) is greater than zero, a
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