1. Why did the Universe Inflate?

2. Proceedings of the Nuffield Workshop, Cambridge, 1982

3. Old Inflation Scenario Time Space Bubble Nucleation Bubble Collision

4. New Inflation Scenario φ Slow roll down Cosmological Constant V

5. Quantum Fluctuations Amplitude [insert equation here] Spectrum [insert equation here]

6. Microwave Background Radiation

7. Why did the Universe Inflate? Why did the scalar field start with a high value of the potential, and run down to a minimum? Why didn’t it just start at the minimum?

8. No boundary amplitude   [h ij,  ]  = Dg e -S[g] Sum over all metrics that have  a boundary and where the induced metric on  is h ij.

9. Wheeler DeWitt Equation -G ijkl δ 2 δh ij δh kl 3 R(h) h ½ + 2Λh ½ Ψ [h ij ] = 0 Where G ijkl is the metric on superspace, G ijkl = ½ h -½ (h ik h jl + h il h jk – h ij h kl ) and 3 R is the scalar curvature of the intrinsic geometry of the three-surface.

10. 1 ∂ 2 1 ∂ 2 ∂a 2 a 2 ∂φ 2 – a 2 – + a 4 V Ψ(a, φ) = 0 Wheeler DeWitt Equation

11. WKB Approximation Ψ = B e iC Δ C·C· Δ C + J = 0 Δ B·B· Δ C = 0

12. No Boundary Amplitude N Amplitude Amplitude = e 1/m 2 N

13. Volume Weighting Surface of present matter density Hubble Volume P( Observing a Hubble Volume ) = | Ψ | 2 × Number of Hubble Volumes MIIMM∞ | Ψ | 2 e 3N Time Space

14. Volume Weighted Probability Initial φ Probability Planck Density Quadratic Potential

15. Volume Weighted Probability Initial φ Probability φ = φ m Potential with a Maximum at φ = φ m

16. Why did the Universe Inflate? Volume weighting gives a high probability of a large amount of Inflation