Perspectives on Galactic Dynamics via General Relativity
F.I. Cooperstock, S. Tieu

TL;DR
This paper defends a general relativistic model of galaxy dynamics, emphasizing its natural description of axially symmetric galaxies and addressing concerns about discontinuities and negative mass layers, supporting the model's physical plausibility.
Contribution
It demonstrates that the galaxy model's discontinuities are physically interpretable and can be resolved without invoking negative mass layers, strengthening the model's validity.
Findings
Discontinuities in the metric derivative relate to density gradients.
Removing the discontinuity yields a continuous density gradient.
Test particle behavior supports the model's physical consistency.
Abstract
Responses to questions, comments and criticism of our recent paper "General Relativity Resolves.." are provided. It is emphasized that our model is entirely natural to describe the dynamics of an axially symmetric galaxy and that our solution, albeit idealized, contains the essence of the problem. The discontinuity of the metric derivative on the symmetry plane is necessarily interpreted as the effect of the mathematically idealized discontinuity of the gradient of the density and is shown to be naturally connected to the distributed volume density via the Gauss divergence theorem. We present arguments to the effect that for our approximate weak field model, we can choose the physically satisfactory mass distribution without an accompanying singular mass surface layer. To support this contention, we modify our solution slightly by removing the discontinuity with a region of continuous…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
