Skip to main content
Book cover

Black Hole Physics

Basic Concepts and New Developments

  • Book
  • © 1998

Overview

Part of the book series: Fundamental Theories of Physics (FTPH, volume 96)

This is a preview of subscription content, log in via an institution to check access.

Access this book

eBook USD 259.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 329.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 329.99
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

Licence this eBook for your library

Institutional subscriptions

Table of contents (17 chapters)

  1. Basic Concepts

  2. Further Developments

  3. Conclusion

Keywords

About this book

It is not an exaggeration to say that one of the most exciting predictions of Einstein's theory of gravitation is that there may exist "black holes": putative objects whose gravitational fields are so strong that no physical bodies or signals can break free of their pull and escape. The proof that black holes do exist, and an analysis of their properties, would have a significance going far beyond astrophysics. Indeed, what is involved is not just the discovery of yet another even if extremely remarkable, astro­ physical object, but a test of the correctness of our understanding of the properties of space and time in extremely strong gravitational fields. Theoretical research into the properties of black holes, and into the possible corol­ laries of the hypothesis that they exist, has been carried out with special vigor since the beginning of the 1970's. In addition to those specific features of black holes that are important for the interpretation of their possible astrophysical manifestations, the theory has revealed a number of unexpected characteristics of physical interactions involving black holes. By the middle of the 1980's a fairly detailed understanding had been achieved of the properties of the black holes, their possible astrophysical manifestations, and the specifics of the various physical processes involved. Even though a completely reliable detection of a black hole had not yet been made at that time, several objects among those scrutinized by astrophysicists were considered as strong candidates to be confirmed as being black holes.

Reviews

`What Frolov and Novikov's book does is present a relatively clear, encyclopedic disussion... its range is impressive... recommend [it] to any graduate student with a grounding in general relativity and an interest in gravitational physics or astrophysics... Frolov and Novikov's book does a very good job in explaing what we know about [black holes] today.'
Physics Today (July 2000)
3

Authors and Affiliations

  • Department of Physics, University of Alberta, Edmonton, Canada

    Valeri P. Frolov

  • Theoretical Astrophysics Center, University of Copenhagen, Copenhagen, Denmark

    Igor D. Novikov

Bibliographic Information

Publish with us