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Primordial Black Holes from String Inflation

5 Pith papers cite this work. Polarity classification is still indexing.

5 Pith papers citing it
abstract

We present a single-field string inflationary model which allows for the generation of primordial black holes in the low mass region where they can account for a significant fraction of the dark matter abundance. The potential is typical of type IIB fibre inflation models and features a plateau at CMB scales and a near inflection point at large distance scales where the power spectrum is enhanced due to a period of ultra slow-roll. The tunability of the underlying parameters is guaranteed by scanning through the string landscape and their stability against quantum corrections is ensured by an effective shift symmetry.

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UV artefacts in ultra-slow-roll models of inflation

astro-ph.CO · 2026-06-26 · unverdicted · novelty 7.0

Hubble-flow models of ultra-slow-roll inflation introduce spurious UV artefacts in the potential that Fourier filtering removes, restoring Wands duality.

Chiral global embedding of Fibre Inflation with $\overline{\rm D3}$ uplift

hep-th · 2024-12-11 · conditional · novelty 7.0

Explicit construction of a chiral global embedding of Fibre Inflation with anti-D3 uplift on an h^{1,1}=4 K3-fibered Calabi-Yau, using magnetised D7-branes, a Whitney brane, and O3-planes at a conifold tip, with viable parameter regions identified.

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  • Chiral global embedding of Fibre Inflation with $\overline{\rm D3}$ uplift hep-th · 2024-12-11 · conditional · none · ref 43 · internal anchor

    Explicit construction of a chiral global embedding of Fibre Inflation with anti-D3 uplift on an h^{1,1}=4 K3-fibered Calabi-Yau, using magnetised D7-branes, a Whitney brane, and O3-planes at a conifold tip, with viable parameter regions identified.