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A small fraction, $f$, of cosmic string loops can collapse to form Primordial Black Holes (PBHs). Constraints on the abundance of PBHs can therefore be used to constrain $f$. We update these calculations, taking into account the PBH extended mass fun
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a79d5ba69e697952b52edacf119d10b2
http://arxiv.org/abs/1911.12658
http://arxiv.org/abs/1911.12658
