Black Holes in Elliptical and Spiral Galaxies and in Globular Clusters

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dc.creatorCahill, Reginald T.
dc.date2005-08-24
dc.date2005-09-22
dc.date.accessioned2026-07-07T06:30:58Z
dc.date.available2026-07-07T06:30:58Z
dc.descriptionSupermassive black holes have been discovered at the centers of galaxies, and also in globular clusters. The data shows correlations between the black hole mass and the elliptical galaxy mass or globular cluster mass. It is shown that this correlation is accurately predicted by a theory of gravity which includes the new dynamics of self-interacting space. In spiral galaxies this dynamics is shown to explain the so-called `dark matter' rotation-curve anomaly, and also explains the earth based bore-hole g anomaly data. Together these effects imply that the strength of the self-interaction dynamics is determined by the fine structure constant. This has major implications for fundamental physics and cosmology.
dc.descriptionLatex, 10 pages, 3 eps figures Additional section re Interpretation and Discussion
dc.identifierhttps://arxiv.org/abs/physics/0508175
dc.identifierhttp://arxiv.org/abs/physics/0508175
dc.identifierProgr.Phys. 3 (2005) 51-56
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98481
dc.subjectGeneral Physics
dc.titleBlack Holes in Elliptical and Spiral Galaxies and in Globular Clusters
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