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

被引：3
|
作者：
Holanda, R. F. L. [1 ,2 ,3 ]
Lima, F. S. [3 ]
Rana, Akshay [4 ]
Jain, Deepak [5 ]
机构：
[1] Univ Fed Rio Grande do Norte, Dept Fis, BR-59072970 Natal, RN, Brazil
[2] Univ Fed Campina Grande, Dept Fis, BR-58429900 Campina Grande, Paraiba, Brazil
[3] Univ Fed Sergipe, Dept Fis, BR-49100000 Aracaju, SE, Brazil
[4] Univ Delhi, St Stephens Coll, Delhi 110007, India
[5] Univ Delhi, Deen Dayal Upadhyaya Coll, New Delhi 110078, India
来源：
EUROPEAN PHYSICAL JOURNAL C | 2022年 / 82卷 / 02期
关键词：
DARK ENERGY; CONSTRAINTS; COSMOLOGY; REPUBLICATION; ASTROPHYSICS; DEFINITION; QUASARS; MASSES;
D O I：
10.1140/epjc/s10052-022-10040-6
中图分类号：
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号：
摘要：
In this paper, we use large scale structure observations to test the redshift dependence of cosmic distance duality relation (CDDR), D-L(1+z)(-2)/D-A = eta(z), with DL and DA, being the luminosity and angular diameter distances, respectively. In order to perform the test, the following data set are considered: strong lensing systems and galaxy cluster measurements (gas mass fractions). No specific cosmological model is adopted, only a flat universe is assumed. By considering two n(z) parametrizations, It is observed that the CDDR remain redshift independent within 1.5 sigma which is in full agreement with other recent tests involving cosmological data. It is worth to comment that our results are independent of the baryon budget of galaxy clusters.
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页数：7
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