The Geometry of Kerr Black Holes by Barrett O'Neill

The Geometry of Kerr Black Holes Barrett O'Neill ebook
Publisher: Dover Publications
Format: pdf
ISBN: 9780486493428
Page: 400

This doesn't apply to a kerr black hole, where you can develop structure within the inner cauchy horizon. €So far, we have If a Kerr black hole rotates too fast, the Kerr black hole becomes a Kerr naked singularity. His work is described in the popular science book, Cracking the Einstein Code by Fulvio Melia. It might give a naked singularity, or perhaps no singularity at all, it has been encountered in . What i mean is that it's not a given that this specific dynamic situation of star "compressing" will end up in the schwarzschild geometry, where we then can use standard black hole reasoning. Nov 13, 2012 - Testing the space-time geometry around black hole candidates with the analysis of the broad K$alpha$ iron line. But then again, that region is unstable. Jan 17, 2012 - But, if the EHT project is successful, it will be the first time a black hole will be directly imaged in any shape or form. Dec 19, 2012 - Professor Kerr has been cited for this work on 'a solution to Einstein's gravitational field equations relating to black holes' in 1963. At least for a schwarzschild black hole.