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Modeling black hole evaporation / Alessandro Fabbri, José Navarro-Salas.

By: Contributor(s): Material type: TextTextPublication details: London : Imperial College Press ; Singapore ; Hackensack, NJ : World Scientific Pub., ©2005.Description: 1 online resource (xiii, 334 pages) : illustrationsContent type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 1860947220
  • 9781860947223
  • 9781860945274
  • 1860945279
Subject(s): Genre/Form: Additional physical formats: Print version:: Modeling black hole evaporation.DDC classification:
  • 523.8/875/015118 22
LOC classification:
  • QB843.B55 F32 2005eb
Online resources:
Contents:
Introduction -- Classical Black Holes -- The Hawking effect -- Near-horizon approximation and conformal symmetry -- Stress tensor, anomalies and effective actions -- Models for eaporating Black Holes.
Summary: The scope of this book is two-fold: the first part gives a fully detailed and pedagogical presentation of the Hawking effect and its physical implications, and the second discusses the backreaction problem, especially in connection with exactly solvable semiclassical models that describe analytically the black hole evaporation process. The book aims to establish a link between the general relativistic viewpoint on black hole evaporation and the new CFT-type approaches to the subject. The detailed discussion on backreaction effects is also extremely valuable.
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Electronic-Books Electronic-Books OPJGU Sonepat- Campus E-Books EBSCO Available

Includes bibliographical references (pages 319-330) and index.

Introduction -- Classical Black Holes -- The Hawking effect -- Near-horizon approximation and conformal symmetry -- Stress tensor, anomalies and effective actions -- Models for eaporating Black Holes.

Print version record.

The scope of this book is two-fold: the first part gives a fully detailed and pedagogical presentation of the Hawking effect and its physical implications, and the second discusses the backreaction problem, especially in connection with exactly solvable semiclassical models that describe analytically the black hole evaporation process. The book aims to establish a link between the general relativistic viewpoint on black hole evaporation and the new CFT-type approaches to the subject. The detailed discussion on backreaction effects is also extremely valuable.

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