Stability of Stellar Systems Orbiting SgrA
Date
2015
Authors
Journal Title
Journal ISSN
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Type
Article
Publisher
arXiv preprint arXiv:1511.02424
Series Info
Doi
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Abstract
Path equations of different orbiting objects in the presence of very strong gravitational fields are essential to examine the impact of its gravitational effect on the
stability of each system. Implementing an analogous method, used to examine the
stability of planetary systems by solving the geodesic deviation equations to obtain
a finite value of the magnitude of its corresponding deviation vectors. Thus, in order
to know whether a system is stable or not, the solution of corresponding deviation
equations may give an indication about the status of the stability for orbiting systems.Accordingly, two questions must be addressed based on the status of stability
of stellar objects orbiting super-massive black holes in the galactic center.
1. Would the deviation equations play the same relevant role of orbiting planetary
systems for massive spinning objects such as neutron stars or black holes?
2. What type of field theory which describes such a strong gravitational field ?
Description
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Keywords
University of Stellar Systems Orbiting; bimetric theory - Path and Path deviation equations; Orbiting particles
Citation
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