On the Extension of the Baryonic Tully-Fisher Relation to Galaxy Clusters and Super Massive-Cosmic Systems

doi:10.4236/oalib.1103686

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Open Access Library Journal 4 2017

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On the Extension of the Baryonic Tully-Fisher Relation to Galaxy Clusters and Super Massive-Cosmic Systems

DOI: 10.4236/oalib.1103686, PP. 1-10

Barbaro Quintero-Leyva

Subject Areas: Mechanics, Modern Physics, Numerical Mathematics

Keywords: Dark Matter, Dark Energy, Galaxies: Kinematics and Dynamics, Clusters, Cosmology

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Abstract

The Baryonic Tully-Fisher relation was extended to clusters hypothesizing that a₀, the characteristic acceleration of the Modified Newtonian Dynamics (MOND), depends on the mass of the system. Circular speeds were calculated for systems with mass up to 10²¹ M_☉. The relativistic impact on super massive systems was considered using the extended Newtonian theory for gravitational bound systems. The impact was an increase of the circular velocity for systems with mass beyond ~10¹⁹ M_☉.

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Quintero-Leyva, B. (2017). On the Extension of the Baryonic Tully-Fisher Relation to Galaxy Clusters and Super Massive-Cosmic Systems. Open Access Library Journal, 4, e3686. doi: http://dx.doi.org/10.4236/oalib.1103686.

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