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Black Hole Physics

From Collapse to Evaporation

  • Highlights the geometrical and quantum information aspects of black holes

  • Focuses on key astronomical observations of black holes, such as the gravitational waves detection

  • Includes a plethora of exercises and tips for solutions

Part of the book series: Graduate Texts in Physics (GTP)

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Table of contents (10 chapters)

  1. Front Matter

    Pages i-xxviii
  2. Introduction

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 1-25
  3. Black Hole Solutions and Basic Properties

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 27-86
  4. Formal Definitions and Classic Theorems

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 87-118
  5. Probing Black Holes, Their Formation and Stability

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 119-145
  6. Black Hole Charges and Thermodynamics

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 147-178
  7. Semiclassical Aspects of Black Holes

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 179-219
  8. Gravity and Black Holes in Diverse Dimensions

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 221-250
  9. Aspects of Holography

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 251-283
  10. Quantum Aspects of Black Holes

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 285-315
  11. Outlook

    • Daniel Grumiller, Mohammad Mehdi Sheikh-Jabbari
    Pages 317-325
  12. Back Matter

    Pages 327-416

About this book

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.

Keywords

  • black hole formation, gravitational collapse and observations
  • black hole horizon and causal structure
  • black hole singularity and area theorems
  • black hole perturbations and stability
  • black hole merger and gravitational wave emission
  • black hole thermodynamics and conserved charges
  • semiclassical aspects of black holes and Hawking radiation
  • asymptotic, near horizon and boundary symmetries
  • black hole evaporation, microstates and information puzzle
  • quantum gravity and black hole holography

Authors and Affiliations

  • Institute for Theoretical Physics, TU Wien, Vienna, Austria

    Daniel Grumiller

  • School of Physics, Institute for Research in Fundamental Sciences, Tehran, Iran

    Mohammad Mehdi Sheikh-Jabbari

About the authors

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.

Bibliographic Information

Buy it now

Buying options

eBook USD 49.99
Price excludes VAT (USA)
  • Available as EPUB and PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 64.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 89.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access