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

partial differential equations with random noise in
SMART_READER_LITE
LIVE PREVIEW

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

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


slide-1
SLIDE 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

slide-2
SLIDE 2

Reheating

  • R. Branden-

berger

Context: The Expanding Universe

Credit: NASA/WMAP Science Team

2 / 13

slide-3
SLIDE 3

Reheating

  • R. Branden-

berger

Optical Telescopes: Gemini Telescope

3 / 13

slide-4
SLIDE 4

Reheating

  • R. Branden-

berger

Galaxies: Building Blocks of the Cosmology

4 / 13

slide-5
SLIDE 5

Reheating

  • R. Branden-

berger

Large-Scale Structure

From: talk by O. Lahav

5 / 13

slide-6
SLIDE 6

Reheating

  • R. Branden-

berger

Power Spectrum of Density Fluctuations

6 / 13

slide-7
SLIDE 7

Reheating

  • R. Branden-

berger

Microwave Telescopes on the Earth: ACT Telescope

7 / 13

slide-8
SLIDE 8

Reheating

  • R. Branden-

berger

Microwave Telescopes on the Earth: SPT Telescope

8 / 13

slide-9
SLIDE 9

Reheating

  • R. Branden-

berger

Microwave Telescopes in Space: WMAP Telescope

9 / 13

slide-10
SLIDE 10

Reheating

  • R. Branden-

berger

Isotropic CMB Background

10 / 13

slide-11
SLIDE 11

Reheating

  • R. Branden-

berger

Map of the Cosmic Microwave Background (CMB)

Credit: NASA/WMAP Science Team

11 / 13

slide-12
SLIDE 12

Reheating

  • R. Branden-

berger

Angular Power Spectrum of CMB Anisotropies

Credit: NASA/WMAP Science Team

12 / 13