Black Hole Physics: From Collapse to Evaporation

ISBN-13: 9783031103421 / Angielski / Twarda / 2022 / 470 str.

Mohammad Mehdi Sheikh-Jabbari

Spis treści

Chapter I: INTRODUCTION

1. A brief review on essentials of General Relativity, from basic concepts, mathematical framework

and Einstein equations Einstein-Hilbert action and classical tests of GR;

2. Brief review of history and timeline of developments from Schwarzschild solution to black hole

mergers and to information paradox and rewall;

3. Gravitational collapse and Chandrasekhar mass bound;

4. Different schools of thought on black holes: high energy oriented, GR oriented and quantum

information theory oriented; open issue how to merge these schools

Chapter II: BASIC CONCEPTS and TOOLS

1. Schwarzschild metric and some basic facts and analysis;

2. Analysis of geodesics, notion of Killing horizon and near horizon Rindler geometry;

3. Kruskal coordinates, maximal extensions and Carter-Penrose diagram;

4. Einstein-Maxwell theory and Reisner-Nordström solution and its basic analysis;

5. Kerr solution and its basic analysis;

6. Black holes in (A)dS backgrounds.

Chapter III: CLASSICAL ASPECTS

1. Lensing and black hole shadows;

2. Super-radiance, Penrose process and black hole mining;

3. Gravitational wave emission in black hole mergers;

4. Accretion disk physics;

5. Extremal black holes, their near horizon and basic analysis.

Chapter IV: ADVANCED CONCEPTS

1. Mathematical defnition of black holes, notion of various different horizons, Killing, event,

cosmological, isolated; trapped surface.

2. Conjectures and theorems (Cosmic censorship; Penrose mass inequality, singularity, uniqueness

and topology theorems)

3. Raychaudhuri equation and area theorem (2nd law); energy conditions;

4. Linear and nonlinear stability of black hole solutions;

5. More detailed analysis of collapse, Choptuik exponents and critical exponents;

6. Canonical boundary charges (1st law), ADM, Brown-York, Regge-Teitelboim, Iyer-Wald-Zoupas,

Barnich-Brandt and Hajian-Sh-J charges.

7. Variation principle; Gibbons-Hawking-York boundary term; Brown-York stress tensor;

8. Quasi-normal modes and black hole perturbations;

9. Four laws of black hole thermodynamics and their new derivations a la Wald-Hajian-Sh-J;

Chapter V: SEMICLASSICAL ASPECTS

1. Quantization on black hole backgrounds;

2. Unruh effect;

3. Hawking effect;

4. Bekenstein entropy and the area law, the Bekenstein bound;

5. Parikh-Wilczek tunneling;

6. Black hole evaporation;

7. Membrane paradigm.

Chapter VI: EXPERT TOPICS

1. Gravity in lower dimensions (including various asymptotic symmetry algebras)

2. Gravity in higher dimensions (including a brief discussion on supergravity);

3. Higher dimensional black hole/ring/brane solutions.

4. Aspects of holography - holographic renormalization, correlation functions and asymptotic

symmetries

5. Extremal black holes and attractor mechanism

6. Kerr/CFT and related topics

7. Soft hair and black hole microstates.

Chapter VII: QUANTUM ASPECTS

1. Black holes in string theory;

2. Microstate counting;

3. Microstate identification/constructions, fuzzballs, fluffballs;

4. Information paradox and black hole complementarity and firewalls;

5. Black holes and quantum gravity;

6. Information paradox and the AdS/CFT;

7. Holography, Quantum information (entanglement entropy, Bousso bound, QNEC etc.) and

generalized laws of black hole thermodynamics.

Chapter VIII: OUTLOOK

1. Summary;

2. Outlook and open issues;

- Experimental/observational prospects

- Black holes as a window to Quantum Gravity

- gravity may be emergent | what does it emerge from?

Chapter IX: SOLUTIONS TO EXERCISES

We present numerous exercises throughout the book and in this chapter we give solutions to a

selected subset of them.

Appendices

We intend to have some appendices in which we present some details of crucial mathematical

frameworks and formulations not fitting into the main text, in particular

- Cartan formulation

- Basics of QFT in curved spacetime

- Covariant phase space method

O autorze

Daniel Grumiller is an Austrian physicist and a Professor at the Institute for Theoretical Physics (ITP) at TU Wien in Vienna. He received his PhD from there in 2001 and joined the ITP faculty in 2009 after postdoc positions at Leipzig U. and MIT. His main research covers black hole holography and "lower-dimensional" gravity, on which he has been lecturing since 2004. His long-term research goal is a comprehensive understanding of quantum gravity, in particular the fate of evaporating black holes and their microscopic structure.

M.M. Sheikh-Jabbari is an Iranian physicist and a Professor at Institute for Research in Fundamental Sciences (IPM) in Tehran. He received his PhD from Sharif Uni. in Tehran in Feb. 1998 and joined IPM as a faculty member in Jan. 2005, after some years of postdoctoral fellowships at IPM, ICTP (Trieste, Italy) and Stanford Uni. His main research covers different areas in Theoretical High Energy Physics, of course including various aspects of black holes, while he has worked on cosmology, in particular the early universe, inflationary models and particle physics phenomenology.

Blurb

This textbook gradually introduces the reader to several topics related to black hole physics with a didactic approach. It starts with the most basic black hole solution, the Schwarzschild metric, and discusses the basic classical properties of black hole solutions as seen by different probes. Then it reviews various theorems about black hole properties as solutions to Einstein gravity coupled to matter fields, conserved charges associated with black holes, and laws of black hole thermodynamics. Next, it elucidates semiclassical and quantum aspects of black holes, which are relevant in ongoing and future research. The book is enriched with many exercises and solutions to assist in the learning.

The textbook is designed for physics graduate students who want to start their research career in the field of black holes; postdocs who recently changed their research focus towards black holes and want to get up-to-date on recent and current research topics; advanced researchers intending to teach (or learn) basic and advanced aspects of black hole physics and the associated mathematical tools. Besides general relativity, the reader needs to be familiar with standard undergraduate physics, like thermodynamics, quantum mechanics, and statistical mechanics. Moreover, familiarity with basic quantum field theory in Minkowski space is assumed. The book covers the rest of the needed background material in the main text or the appendices.