Beyond Einstein:
From the Big Bang to Black Holes

Stanford Linear Accelerator Center,

Stanford University, 12-15 May 2004

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Introduction to General Topology in the Study of Orbits in the Galactics Nuclei

Ricardo Godano
 
rgodano@yahoo.com

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The present I work tries to explain some concepts related to the orbits and its components. In the same one three types will be analyzed of orbits: a. Keplerian orbits: those that comply with the three laws of Kepler and do not possess irregularities. b. Relativist orbits: those that comply the bases of the General Theory of the Relativity, and present precesion of periastro. c. Chaotics orbits: those that are originated they go the problem of the n bodies and the points of Lagrange. Especially in the last category of orbits, they will apply the concepts of the General Topology to determine stable components of said orbits. The calculations that will apply in this category will be referred to the star S2 that orbit around the Supermass Black Hole of the Center of our Milky Way.

 

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