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E-raamat: Advanced Lectures on General Relativity

  • Formaat: EPUB+DRM
  • Sari: Lecture Notes in Physics 952
  • Ilmumisaeg: 31-Jan-2019
  • Kirjastus: Springer Nature Switzerland AG
  • Keel: eng
  • ISBN-13: 9783030042608
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Advanced Lectures on General RelativitySuurem pilt
  • Formaat: EPUB+DRM
  • Sari: Lecture Notes in Physics 952
  • Ilmumisaeg: 31-Jan-2019
  • Kirjastus: Springer Nature Switzerland AG
  • Keel: eng
  • ISBN-13: 9783030042608
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These lecture notes are intended for starting PhD students in theoretical physics who have a working knowledge of General Relativity. The four topics covered are:
  1. Surface charges as conserved quantities in theories of gravity;
  2. Classical and holographic features of three-dimensional Einstein gravity;
  3.  Asymptotically flat spacetimes in four dimensions: BMS group and memory effects;
  4. The Kerr black hole: properties at extremality and quasi-normal mode ringing.
Each topic starts with historical foundations and points to a few modern research directions.

Arvustused

In accordance with the authors aim to target young PhD students in physics or postdocs, these lecture notes have definitely been written in the language and style of physicists. (Gabor Etesi, zbMath 1419.83003, 2019)

Surface charges in Gravitation.- Three dimensional Einstein gravity.- Asymptotically flat spacetime.- Rotating black holes.
Geoffrey Compère is a FNRS Research Associate at the Université Libre de Bruxelles, Belgium. His research, as a theoretical physicist, focuses on surface charges in gravitation, the physics of black holes close to extremality, supergravity and infinite-dimensional symmetries, topics on which he has authored over 50 papers. He developed the package SurfaceCharges for Mathematica which allows to compute surface charges in gravitation coupled to matter. He is the recipient of an ERC Starting Grant addressing the holographic properties of black holes. As a member of the LISA consortium and of the Belgian Gravitational Wave Center, he is currently developing waveform models to confront General Relativity with upcoming high-precision gravitational wave observations.
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