On the Gravitomagnetic Origins of the Spiral Character of Galaxies

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dc.contributor.authorNyambuya, G. G.
dc.date.accessioned2018-07-04T10:44:36Z
dc.date.accessioned2023-06-26T13:01:59Z
dc.date.available2018-07-04T10:44:36Z
dc.date.available2023-06-26T13:01:59Z
dc.date.issued2018-05
dc.descriptionArticleen_US
dc.description.abstractWe here demonstrate that the proposed hitherto unknown gravitomagnetic dark-force (Nyambuya 2018) that hypothetically explains the Flat Rotation Curves of Spiral Galaxies – this same force, explains very well, the logarithmic spiral shapes of spiral galaxies. The galactic disk is here assumed to be in a state of free-fall around the central bulge with the hypothetical gravitomagnetic dark-force being the dominate force determining all gravity-related dynamics of the disk.en_US
dc.identifier.citationNyambuya, G. G. 2018. On the Gravitomagnetic Origins of the Spiral Character of Galaxies. [Online] available from: https://www.researchgate.net/publication/325343821. [Accessed on: 13/06/8]en_US
dc.identifier.other10.13140/RG.2.2.34396.49288
dc.identifier.urihttp://ir.nust.ac.zw:4000/handle/123456789/917
dc.language.isoen_USen_US
dc.publisherResearchGateen_US
dc.subjectdarkmatteren_US
dc.subjectgravitatomagnetismen_US
dc.subjectTully-Fisher relationen_US
dc.subjectgalaxy rotation curves.en_US
dc.titleOn the Gravitomagnetic Origins of the Spiral Character of Galaxiesen_US
dc.typeArticleen_US

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