Black Hole Astrophysics

Part I Observations of Black Hole Engines

1 Recognizing Black Holes

2 Macroquasars: Supermassive Black Holes in the Centers of Galaxies

3 Microquasars: Black holes (and Neutron Stars) of Stellar Mass in Our Galaxy

4 Miniquasars: Elusive Black Holes of Intermediate Mass

Part II Physics of Black Hole Engines

5 Physics in Everyday Life: A Review of Newtonian Mechanics

6 Geometry and Physics Without Gravity: Special Relativity

7 Physics in Curved Spacetime: General Relativity and Black Holes

8 Four-Dimensional Evolving Geometry: Gravitational Waves and Gravitational Collapse

9 Nuts and Bolts of the Black Hole Engine: General Relativistic Mechanics

Part III Astrophysics of Black Hole Engines

10 Assembling the Engine Block: Formation of Black Holes in the Universe

11 Fueling and Carburetion: Breakup and Accretion of Stars and Gas Clouds

12 The Combustion Chamber: Energy Generation by Gravitational Accretion

13 The Thermal Exhaust System: Radiation and Thermally-Driven Winds

14 The Non-Thermal Exhaust System I. Rotating Magnetospheres: The Fan that Drives the Turbo-Exhaust System

15 The Non-Thermal Exhaust System II. Magnetic Winds and Jets

16 Putting it All Together: Black Hole Engines of All Sizes

Part IV Appendices

A Mathematical Notation Used in this Book

B Derivatives of Vectors and Tensors: Differential Geometry

C Derivation of the Adiabatic Relativistic Stellar Structure Equations

D Derivation of the General Relativistic MHD Equations from Kinetic Theory

E Derivation of the General Relativistic Grad-Schlüter-Shafranov Equation

F Derivation of the Equations for Stationary, Axisymmetric Ideal MHD

References

David Meier is a Senior Research Scientist and supervisor of the Evolution of Galaxies Group at Caltech's Jet Propulsion  Laboratory in Pasadena, CA.  David had an early career doing research in genetics at Washington University School of Medicine and in solid state physics at the University of Missouri - Rolla (UMR), before achieving his goal of research in astrophysics. He was educated in physics at UMR (BS 1971; MS 1973) and in astrophysics at The University of Texas at Austin (MA 1975; PhD 1977), working there under D. Schramm, B. Tinsley, and J.C. Wheeler on astrophysical jet production, galaxy formation, and winds from accretion disks around black holes.  In 1976, with Tinsley, he predicted the existence of primeval Lyman break galaxies, which since have been discovered and found to have many of their expected properties.  At Caltech and JPL David has been an integral part of a number of projects and missions involving observations of galaxies and black hole systems, including very long baseline radio interferometry (VLBI) in the southern hemisphere, VLBI using a space-based antenna (which created a telescope three times the size of the earth), and the space interferometer mission SIM.  He also spent several years working on the US government's "star wars" project and was the group leader for parallel computing applications in that effort.  While much of his recent work has been theoretical investigations of accretion inflows and outflows from black holes systems, David also enjoys occasional observational studies, using some of the satellites and telescopes on which he has worked. He also greatly enjoys his three grandsons, with a fourth soon to arrive.

 

From the reviews:"This gigantic and outstanding book summarizes the state of the art of black hole physics. ... The mathematical presentation is didactically excellent. ... The chapters about the exhaust systems are a further highlight of the book. The different mechanisms are clearly explained and judged ... . The book can be sincerely recommended for all astrophysical tutorials and to all students engaged in astrophysics." (Johannes Viktor Feitzinger, Zentralblatt MATH, Vol. 1259, 2013)