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The Cosmic Microwave Background: Relevance and Anisotropies in Observational Cosmology

The Cosmic Microwave Background: Relevance and Anisotropies in Observational Cosmology

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

Introduction

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1 of 14

Introduction

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Classroom Contents

The Cosmic Microwave Background: Relevance and Anisotropies in Observational Cosmology

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  1. 1 Introduction
  2. 2 Background History
  3. 3 Background Prediction
  4. 4 The History of the Universe
  5. 5 Nuclear Synthesis
  6. 6 Dark Ages
  7. 7 Why are there fluctuations
  8. 8 CMP
  9. 9 Data
  10. 10 Angular Scale
  11. 11 Parameters
  12. 12 Hubble parameter
  13. 13 Polarization
  14. 14 Conclusion

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