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Applying modified gravity to the lensing and Einstein ring in Abell 3827

J. W. MoffatDepartment of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, CanadaViktor T. TothPerimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
2021en
ABI

Abstract

The lensing and Einstein ring at the core of the galaxy cluster Abell 3827 are reproduced in the modified gravity theory (MOG). The estimated effective lensing mass ${M}_{L}=(1+\ensuremath{\alpha}){M}_{b}=5.2\ifmmode\times\else\texttimes\fi{}{10}^{12}\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ within $R=18.3\text{ }\text{ }\mathrm{kpc}$ for a baryon mass ${M}_{b}=1.0\ifmmode\times\else\texttimes\fi{}{10}^{12}\text{ }\text{ }{M}_{\ensuremath{\bigodot}}$ within the same radius produces the observed Einstein ring angular radius ${\ensuremath{\theta}}_{E}=1{0}^{\ensuremath{'}\ensuremath{'}}$. A detailed derivation of the total lensing mass is based on modeling of the cluster configuration of galaxies, intracluster light and x-ray emission. The MOG can fit the lensing and Einstein ring in Abell 3827 without dark matter as well as general relativity with dark matter.

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