Beyond Black Holes: Uniqueness Properties of Ultra-Massive Spacetimes - Lecture

Beyond Black Holes: Uniqueness Properties of Ultra-Massive Spacetimes - Lecture

Erwin Schrödinger International Institute for Mathematics and Physics (ESI) via YouTube Direct link

Simple spherical symmetric models

3 of 16

3 of 16

Simple spherical symmetric models

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Beyond Black Holes: Uniqueness Properties of Ultra-Massive Spacetimes - Lecture

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  1. 1 Introduction
  2. 2 Cosmodial constant
  3. 3 Simple spherical symmetric models
  4. 4 Ultramassive models
  5. 5 Basic notion
  6. 6 Terminology
  7. 7 The Cutler Metric
  8. 8 Standard black hole
  9. 9 Collapsing universe
  10. 10 Black hole formation
  11. 11 Normal situation
  12. 12 External directions
  13. 13 Stability operator
  14. 14 Ultramassive spacetime
  15. 15 Universal properties
  16. 16 Implications

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