The Galactic Black Hole Lectures on General Relativity and Astrophysics

Date: 19 January 2011, 09:00

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The supermassive black hole in the center of our Milky Way is the nearest such object and relatively easy to observe and study. Not surprisingly therefore, it is the best studied supermassive black hole. Many astrophysical and even general relativistic effects can be investigated in great detail. These lectures provide a systematic introduction to the physics/astrophysics and mathematics of black holes at a level suitable for graduate students, postdocs and researchers in physics, astrophysics, astronomy, and applied mathematics. The focus is mainly on the supermassive black hole in the center of our Milky Way but the results can be easily generalised taking it as an example. Leading international experts provide first hand accounts of the observational and theoretical aspects of this black hole. Topics range from the properties of the Schwarzschild metric and the collapse to a black hole, to quantum gravity; and from the structure of the Galaxy to accretion of matter and the emission properties of the Galactic Center black hole.

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