A Guide to Black Holes


Kenath Arun, PhD – Assistant Professor, Department of Physics & Electronics, CHRIST (Deemed to be University), Bengaluru, India

Series: Space Science, Exploration and Policies
BISAC: SCI015000
DOI: 10.52305/TKOH1520

The idea of a black hole goes back to Laplace or maybe even earlier to Englishman John Michell, referring to these bodies as ‘dark stars’, way back in 1783. Laplace argued that the largest objects in the universe must become invisible and would hence be dark. When Einstein proposed his general theory of relativity in the early 1900s, Schwarzschild solved the equation (1916) for a spherical star and the solution implied that below a radius (referred to as the Schwarzschild radius), all light and other radiation are trapped inside the star, and it becomes what is called a black hole. With better detection mechanisms, such as the images from the Event Horizon Telescope, the universe of black holes is opening up for astronomical observations and discoveries over all wavelengths. This book covers a wide range of topics related to black holes and their dynamics.

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Table of Contents


Chapter 1. Invoking Dark Matter in the Formation of SMBH in the Very Early Universe: A Possible Solution to a Continuing Conundrum
Arun Kenath¹ and C. Sivaram²
¹CHRIST (Deemed to be University), Bangalore, India
²Indian Institute of Astrophysics, Bangalore, India

Chapter 2. Quantum Black Holes and their Applications to a QFT Applicability Boundary Investigation
Alexander E. Shalyt-Margolin
Institute for Nuclear Problems, Belarusian State University, Minsk, Belarus

Chapter 3. Thermodynamics of Black Hole and Thermal Fluctuations
Dr. Sudhaker Upadhyay
Department of Physics, K. L. S. College, Nawada, Bihar, India; Department of Physics, Magadh University, Bodh Gaya, Bihar, India

Chapter 4. Motion of Spinning Particles around Black Holes
Jose Miguel Ladino
Universidad Nacional de Colombia, Sede BogotÃ, Facultad de Ciencias, Observatorio Astronà mico Nacional, Ciudad Universitaria, Bogota, Colombia

Chapter 5. Testing a Microscopic Model for Black Holes Deduced from Maximum Force
Christoph Schiller
Motion Mountain Research, Munich, Germany

Chapter 6. From Bohr to Schrodinger: A Two-Particle System Approach to Black Hole Quantum Gravity
Christian Corda
International Institute for Applicable Mathematics and Information Sciences, B. M. Birla Science Centre, Adarshnagar, Hyderabad, India; Istituto Livi, Via Antonio Marini, Prato, Italy

Chapter 7. Black Hole Menagerie, Charged/Dyonic BHs and Radiation from Interacting Dyonic BH Pairs
Patrick Das Gupta and Mohd. Sirtaz
Department of Physics and Astrophysics, University of Delhi, Delhi, India