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If the inflaton gets trapped in a local minimum of its potential shortly before the end of inflation, it escapes by building up quantum fluctuations in a process known as stochastic tunnelling.
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D. Wands, K. A. Malik, D. H. Lyth and A. R. Liddle, A New approach to the evolution of cosmological perturbations on large scales , Phys. Rev. D 62
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V. Vennin and A. A. Starobinsky, Correlation Functions in Stochastic Inflation , Eur. Phys. J. C 75
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“ NIST Digital Library of Mathematical Functions
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