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Title: Significance of Gravitational Nonlinearities on the Dynamics of Disk Galaxies
The discrepancy between the visible mass in galaxies or galaxy clusters, and that inferred from their dynamics is well known. The prevailing solution to this problem is dark matter. Here we show that a different approach, one that conforms to both the current Standard Model of Particle Physics and General Relativity, explains the recently observed tight correlation between the galactic baryonic mass and its observed acceleration. Using direct calculations based on General Relativity's Lagrangian, and parameter-free galactic models, we show that the nonlinear effects of General Relativity make baryonic matter alone sufficient to explain this observation.  more » « less
Award ID(s):
1847771
NSF-PAR ID:
10157235
Author(s) / Creator(s):
; ;
Date Published:
Journal Name:
The Astrophysical journal
ISSN:
2471-4259
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
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