Hybrid -attractors, primordial black holes and gravitational wave backgrounds
arXiv:2211.14262 · doi:10.1088/1475-7516/2023/04/033
Abstract
We investigate the two-stage inflation regime in the theory of hybrid cosmological -attractors. The spectrum of inflationary perturbations is compatible with the latest Planck/BICEP/Keck results, thanks to the attractor properties of the model. However, at smaller scales, it may have a very high peak of controllable width and position, leading to a copious production of primordial black holes (PBH) and generation of a stochastic background of gravitational waves (SGWB).
39 pages, 12 figures, v2: references added, minor modifications, matches JCAP version
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