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    Is the formation of primordial black holes from single-field inflation compatible with standard cosmology?

    Sasha Allegrini1,*, Loris Del Grosso1,2,3,†, Antonio J. Iovino1,2,4,‡, and Alfredo Urbano1,2,§

    • *Contact author: allegrini.2082804@studenti.uniroma1.it
    • †Contact author: loris.delgrosso@uniroma1.it
    • ‡Contact author: antoniojunior.iovino@uniroma1.it
    • §Contact author: alfredo.urbano@uniroma1.it

    Phys. Rev. D 111, 123557 – Published 27 June, 2025

    DOI: https://doi.org/10.1103/9rr3-ltbt

    Abstract

    In this work, we investigate the generation of primordial black holes (PBHs) within the framework of single-field inflationary models and their compatibility with the cosmological history of the Universe. Our results suggest that, depending on the masses of the formed PBHs, single-field inflation models require more than fine-tuning a potential to induce ultraslow roll; it necessitates a comprehensive understanding of the postinflationary cosmological evolution. As an explicative example, we introduce a new model, based on a double inflection point and consistent with cosmic microwave background observations, capable of generating subsolar PBHs, whose merger could be potentially detectable by the LVK experiment.

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