Black Holes A Laboratory For Testing Strong Gravity
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Black Holes: A Laboratory for Testing Strong Gravity
This textbook introduces the current astrophysical observations of black holes, and discusses the leading techniques to study the strong gravity region around these objects with electromagnetic radiation. More importantly, it provides the basic tools for writing an astrophysical code and testing the Kerr paradigm. Astrophysical black holes are an ideal laboratory for testing strong gravity. According to general relativity, the spacetime geometry around these objects should be well described by the Kerr solution. The electromagnetic radiation emitted by the gas in the inner part of the accretion disk can probe the metric of the strong gravity region and test the Kerr black hole hypothesis. With exercises and examples in each chapter, as well as calculations and analytical details in the appendix, the book is especially useful to the beginners or graduate students who are familiar with general relativity while they do not have any background in astronomy or astrophysics.“/p>
Artificial Black Holes
Physicists are pondering on the possibility of simulating black holes in the laboratory by means of various OC analog modelsOCO. These analog models, typically based on condensed matter physics, can be used to help us understand general relativity (Einstein''s gravity); conversely, abstract techniques developed in general relativity can sometimes be used to help us understand certain aspects of condensed matter physics. This book contains 13 chapters OCo written by experts in general relativity, particle physics, and condensed matter physics OCo that explore various aspects of this two-way traffic."
From X-ray Binaries to Quasars: Black Holes on All Mass Scales
Author: Thomas J. Maccarone
language: en
Publisher: Springer Science & Business Media
Release Date: 2007-01-28
This volume brings together contributions from many of the world's leading authorities on black hole accretion. The papers within represent part of a new movement to make use of the relative advantages of studying stellar mass and supermassive black holes and to bring together the knowledge gained from the two approaches. The topics discussed here run the gamut of the state of the art in black hole observational and theoretical work-variability, spectroscopy, disk-jet connections, and multi-wavelength campaigns on black holes are all covered. Reprinted from ASTROPHYSICS AND SPACE SCIENCE, 300:1-3 (2005)