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Partial Differential Equations with Random Noise in Inflationary - PowerPoint PPT Presentation

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Reheating R. Branden- berger Partial Differential Equations with Random Noise in Inflationary Cosmology Effects of Noise on Preheating Robert Brandenberger, McGill University January 11, 2014 1 / 13 Context: The Expanding Universe

  1. Reheating R. Branden- berger Partial Differential Equations with Random Noise in Inflationary Cosmology Effects of Noise on Preheating Robert Brandenberger, McGill University January 11, 2014 1 / 13

  2. Context: The Expanding Universe Reheating R. Branden- berger Credit: NASA/WMAP Science Team 2 / 13

  3. Optical Telescopes: Gemini Telescope Reheating R. Branden- berger 3 / 13

  4. Galaxies: Building Blocks of the Cosmology Reheating R. Branden- berger 4 / 13

  5. Large-Scale Structure Reheating R. Branden- berger From: talk by O. Lahav 5 / 13

  6. Power Spectrum of Density Fluctuations Reheating R. Branden- berger 6 / 13

  7. Microwave Telescopes on the Earth: ACT Telescope Reheating R. Branden- berger 7 / 13

  8. Microwave Telescopes on the Earth: SPT Telescope Reheating R. Branden- berger 8 / 13

  9. Microwave Telescopes in Space: WMAP Telescope Reheating R. Branden- berger 9 / 13

  10. Isotropic CMB Background Reheating R. Branden- berger 10 / 13

  11. Map of the Cosmic Microwave Background (CMB) Reheating R. Branden- berger Credit: NASA/WMAP Science Team 11 / 13

  12. Angular Power Spectrum of CMB Anisotropies Reheating R. Branden- berger Credit: NASA/WMAP Science Team 12 / 13

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