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Black Holes in Elliptical and Spiral Galaxies and in Globular Clusters

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dc.creator Cahill R. T.
dc.date 2005
dc.date.accessioned 2013-06-01T12:21:05Z
dc.date.available 2013-06-01T12:21:05Z
dc.date.issued 2013-06-01
dc.identifier http://www.ptep-online.com/index_files/2005/PP-03-09.PDF
dc.identifier http://www.doaj.org/doaj?func=openurl&genre=article&issn=15555534&date=2005&volume=3&issue=&spage=51
dc.identifier.uri http://koha.mediu.edu.my:8181/jspui/handle/123456789/8831
dc.description Supermassive 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.publisher HEXIS (Arizona, USA)
dc.source Progress in Physics
dc.subject Classical Mechanics
dc.subject Astrophysics
dc.title Black Holes in Elliptical and Spiral Galaxies and in Globular Clusters

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