PPT Slide

Developing Warm Inflation

Observations

Theory

• Thermal perturbations, amplitude & slope

• Tensor modes

• Super-Hubble suppression

• Isothermal perturbations

• Primary & secondary acoustic peaks.

• Non-Gaussian signatures.

• Dissipative QFT at low temp, and out of equilibrium.

• Particle physics models.

• Implications for magnetic fields / baryogensis.

• Robustness of solutions.

MAP, Planck polarization will supply vast data in coming years.

General physics developed from this study:

- first principles Landau-Ginzburg dynamics.

- New tests of CMBR.

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