Author:
Ghosh Shubhrangshu,Bhattacharya Mahasweta,Sherpa Yanzi,Bhadra Arunava
Abstract
Abstract
Weyl's conformal gravity theory, which is considered as a compelling alternative to
general relativity theory, has been claimed to describe the observed flat rotation curve feature
of spiral galaxies without the need of invoking dark matter. However, it is important to examine
whether the Weyl theory can also explain the relevant gravitational lensing observations correctly
without considering any dark matter. In this regard, the gravitational bending angle in static
spherically space-time (Mannheim-Kazanas metric) in Weyl theory has been calculated by several
authors over the last two decades, but the results are found largely divergent. In this work, we
have revisited the problem and obtain the correct and consistent expression of the deflection
angle in conformal gravity. Subsequently we perform the gravitational lensing analysis. We compare
the prediction of Weyl gravity with the gravitational lensing observations of the rich galaxy
clusters Abell 370 and Abell 2390 and is found that Weyl theory cannot describe the stated lensing
observations without considering dark matter.
Subject
Astronomy and Astrophysics
Cited by
1 articles.
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