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2014

Universality classes for models of inflation

Binetruy, P., Kiritsis, E., Mabillard, J. et al.

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We show that the cosmological evolution of a scalar field in a potential can be obtained from a renormalisation group equation.

The slow roll regime of inflation models is understood in this context as the slow evolution close to a fixed point, described by the methods of renormalisation group.
This explains in part the universality observed in the predictions of a certain number of inflation models.
We illustrate this behavior on a certain number of examples and discuss it in the context of the AdS/CFT correspondence.

Universality classes for models of inflation · Around

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