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Running-Mass Inflation Model and Primordial Black Holes · Around

2011

Running-Mass Inflation Model and Primordial Black Holes

Drees, Manuel, Erfani, Encieh

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We revisit the question whether the running-mass inflation model allows the formation of Primordial Black Holes (PBHs) that are sufficiently long-lived to serve as candidates for Dark Matter.

We incorporate recent cosmological data, including the WMAP 7-year results.
Moreover, we include "the running of the running" of the spectral index of the power spectrum, as well as the renormalization group "running of the running" of the inflaton mass term.
Our analysis indicates that formation of sufficiently heavy, and hence long-lived, PBHs still remains possible in this scenario.

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