Primordial black holes from string inflation
By M. Cicoli, V. A. Diaz, F. Pedro. Journal of Cosmology and Astroparticle Physics, 2018
150 citations recorded by the source corpus.
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 small distance scales where the power spectrum is enhanced due to a period of ultra slow-roll. The tunability of the underlying parameters may be guaranteed by scanning through the string landscape and their stability against quantum corrections is ensured by an effective shift symmetry.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/da5889878b7ab9e94b1dbe5b2b982fe43a336c84
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Citations in the corpus
- Primordial black holes from α-attractors (2018, background): “Critical Higgs inflation [20], simple polynomials or potentials with a radiative plateau a la Coleman-Weinberg where the inflaton is non-minimally coupled to the Ricci scalar [21, 22], fibre inflation [24] and axion models [25] inspired by string theory, supergravity [26] are examples of single fiel”
- Primordial black holes from inflation and quantum diffusion (2018, methodology): “[18] with parameter set defined in Tab 1.”
- Generating PBHs and small-scale GWs in two-field models of inflation (2020, background): “This can be achieved in single-field inflation scenarios by using a local feature in the inflaton potential like a rapid change of its amplitude or a break in its first derivative [7–9], an inflection point [10–18] or a tiny bump superimposed on it [19, 20], non-trivial inflaton sound speed [21–23]1”
- Mechanisms for primordial black hole production in string theory (2018, unknown): “For example, an attempt towards embedding this model within string theory via fine-tuned string-loop corrections in fibre inflation has been made very recently in [12], although it has not yet proved possible to fine-tune a setup such that cosmological (1)A possible obstacle for PBH’s as Dark Matter”