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Cosmological Perturbations from Non-Equilibrium Quantum Fields

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Cosmic Microwave Background<br />

Highly Gaussian −10 < f NL < 74 (i.e. ζ NG 10 −8 )<br />

Nearly scale-invariant spectrum n s = 0.963 ± 0.012<br />

Just as inflation predicts!<br />

Arttu Rajantie<br />

<strong>Cosmological</strong> <strong>Perturbations</strong> <strong>from</strong> <strong>Non</strong>-<strong>Equilibrium</strong> <strong>Quantum</strong> <strong>Fields</strong> – SEWM 2012

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