Black hole physics : from collapse to evaporation / Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari.

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Sonraí bibleagrafaíochta
Príomhchruthaitheoirí: Grumiller, Daniel (Údar), Sheikh-Jabbari, Mohammad Mehdi (Údar)
Formáid: Ríomhleabhar
Teanga:English
Foilsithe / Cruthaithe: Cham : Springer, [2022]
Sraith:Graduate texts in physics.
Ábhair:
Rochtain ar líne:Click for online access
Clár na nÁbhar:
  • Intro
  • Foreword
  • Preface
  • How to Read and Use This Book
  • Acknowledgements
  • Contents
  • Acronyms
  • Notations and Conventions
  • List of Figures
  • 1 Introduction
  • 1.1 Essentials of General Relativity
  • 1.1.1 Equivalence Principle and Geodesics
  • 1.1.2 Einstein Gravity
  • 1.2 Brief Review of Black Hole History
  • 1.2.1 First Five Decades: Finding Solutions and Classic Analyses
  • 1.2.2 Black Holes Through Observations
  • 1.2.3 Black Holes as Thermodynamical Systems
  • 1.3 Gravitational Collapse in Stars
  • 1.3.1 Core Collapse Supernova and Black Hole Formation
  • 1.3.2 Estimating the Chandrasekhar Mass
  • 1.4 Different Schools of Thought on Black Holes
  • 1.4.1 GR School
  • 1.4.2 HEP School
  • 1.4.3 Quantum Information School
  • 2 Black Hole Solutions and Basic Properties
  • 2.1 Schwarzschild Metric, Basic Facts, and Analyses
  • 2.1.1 Symmetries and Killing Vectors
  • 2.1.2 Flamm Diagram
  • 2.1.3 Singularities, Asymptotic, and Near Horizon Behavior
  • 2.1.4 ADM Mass and Angular Momentum
  • 2.1.5 Infinite Redshift Surface
  • 2.2 Particle Probes and Geodesics
  • 2.2.1 Null Geodesics
  • 2.2.2 Timelike Geodesics and Particle Orbits
  • 2.2.3 Eddington-Finkelstein Coordinates
  • 2.3 Maximal Extensions and Causal Diagrams
  • 2.3.1 Geodesic Completeness and Maximal Analytic Extension
  • 2.3.2 Kruskal Coordinates for Schwarzschild Geometry
  • 2.3.3 Structure of Lightcones and Preliminary Notion of Horizon
  • 2.3.4 Carter-Penrose Causal Diagrams
  • 2.3.5 Realistic Black Holes and Wormholes
  • 2.4 Einstein-Maxwell Theory and Reissner-Nordström Black Holes
  • 2.5 Kerr Solution and Its Basic Analysis
  • 2.5.1 Basic Properties of Kerr Black Hole
  • 2.5.2 Geodesics of Kerr Geometry
  • 2.6 Black Holes in (A)dS Backgrounds
  • 2.6.1 Schwarzschild-dS Black Holes
  • 2.6.2 Schwarzschild-AdS and Topological Black Holes
  • 2.7 Plebanski-Demianski Black Holes
  • 2.8 Vaidya Metric as Example for Non-stationary Black Holes
  • 3 Formal Definitions and Classic Theorems
  • 3.1 Mathematical Definitions of Black Holes and Horizons
  • 3.1.1 Killing Horizon and Surface Gravity
  • 3.1.2 Event Horizon and Mathematical Black Hole Definition
  • 3.1.3 Apparent Horizons and Trapped Surfaces
  • 3.1.4 Cauchy Horizons and Predictability
  • 3.1.5 Other Horizon Definitions
  • 3.2 Classic Conjectures and Theorems
  • 3.2.1 Raychaudhuri Equation
  • 3.2.2 Classical Energy Conditions
  • 3.2.3 Singularity Theorems
  • 3.2.4 Asymptotic Flatness
  • 3.2.5 Horizon Theorems
  • 3.2.6 Uniqueness Theorems
  • 3.2.7 Cosmic Censorship Conjecture
  • 3.3 Optical Focusing Equation and Area Theorem (2nd Law)
  • 4 Probing Black Holes, Their Formation and Stability
  • 4.1 General Remarks on Black Hole Observations
  • 4.2 Black Hole Photon-Sphere, Shadows, and Images
  • 4.3 Penrose Process, Super-Radiance, and Black Hole Mining
  • 4.4 Gravitational Waves and Black Hole Mergers
  • 4.5 Accretion Disk Physics
  • 4.6 Black Hole Formation in Shock-Wave Collisions