The MOG Weak Field approximation II. Observational test of Chandra X-ray Clusters
The MOG Weak Field approximation II. Observational test of Chandra X-ray Clusters
About this item
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Author / Creator
Moffat, J W and Rahvar, S
Publisher
Ithaca: Cornell University Library, arXiv.org
Journal title
Language
English
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Publisher
Ithaca: Cornell University Library, arXiv.org
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Scope and Contents
Contents
We apply the weak field approximation limit of the covariant Scalar-Tensor-Vector Gravity (STVG) theory, so-called MOdified gravity (MOG), to the dynamics of clusters of galaxies by using only baryonic matter. The MOG effective gravitational potential in the weak field approximation is composed of an attractive Newtonian term and a repulsive Yukawa...
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Full title
The MOG Weak Field approximation II. Observational test of Chandra X-ray Clusters
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Record Identifier
TN_cdi_proquest_journals_2082697478
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2082697478
Other Identifiers
E-ISSN
2331-8422
DOI
10.48550/arxiv.1309.5077
