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Primordial black holes and inflation from double-well potentials

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Primordial black holes and inflation from double-well potentials. / Karam, Alexandros; Koivunen, Niko; Tomberg, Eemeli et al.
In: Journal of Cosmology and Astroparticle Physics, Vol. 2023, No. 9, 002, 01.09.2023.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Karam, A, Koivunen, N, Tomberg, E, Racioppi, A & Veermäe, H 2023, 'Primordial black holes and inflation from double-well potentials', Journal of Cosmology and Astroparticle Physics, vol. 2023, no. 9, 002. https://doi.org/10.1088/1475-7516/2023/09/002

APA

Karam, A., Koivunen, N., Tomberg, E., Racioppi, A., & Veermäe, H. (2023). Primordial black holes and inflation from double-well potentials. Journal of Cosmology and Astroparticle Physics, 2023(9), Article 002. https://doi.org/10.1088/1475-7516/2023/09/002

Vancouver

Karam A, Koivunen N, Tomberg E, Racioppi A, Veermäe H. Primordial black holes and inflation from double-well potentials. Journal of Cosmology and Astroparticle Physics. 2023 Sept 1;2023(9):002. doi: 10.1088/1475-7516/2023/09/002

Author

Karam, Alexandros ; Koivunen, Niko ; Tomberg, Eemeli et al. / Primordial black holes and inflation from double-well potentials. In: Journal of Cosmology and Astroparticle Physics. 2023 ; Vol. 2023, No. 9.

Bibtex

@article{71cf9b903b1040c9abe4297132541ab5,
title = "Primordial black holes and inflation from double-well potentials",
abstract = "We investigate the formation of large peaks in the inflationary curvature power spectrum from double-well potentials. In such scenarios, the initial CMB spectrum is created at large field values. Subsequently, the inflaton will cross one of the minima and will decelerate rapidly as it reaches the local maximum at the origin, either falling back or crossing it. During this final phase, a significant peak in the curvature power spectrum can be generated. Our analysis reveals that this class of models produces more pronounced peaks than most quasi-inflection point scenarios with less tuning for the model parameters. Finally, we construct an explicit theoretically motivated inflationary scenario that is consistent with the latest CMB observations and capable of generating sufficiently large curvature perturbations for primordial black holes.",
keywords = "inflation, primordial black holes",
author = "Alexandros Karam and Niko Koivunen and Eemeli Tomberg and Antonio Racioppi and Hardi Veerm{\"a}e",
year = "2023",
month = sep,
day = "1",
doi = "10.1088/1475-7516/2023/09/002",
language = "English",
volume = "2023",
journal = "Journal of Cosmology and Astroparticle Physics",
issn = "1475-7516",
publisher = "IOP Publishing",
number = "9",

}

RIS

TY - JOUR

T1 - Primordial black holes and inflation from double-well potentials

AU - Karam, Alexandros

AU - Koivunen, Niko

AU - Tomberg, Eemeli

AU - Racioppi, Antonio

AU - Veermäe, Hardi

PY - 2023/9/1

Y1 - 2023/9/1

N2 - We investigate the formation of large peaks in the inflationary curvature power spectrum from double-well potentials. In such scenarios, the initial CMB spectrum is created at large field values. Subsequently, the inflaton will cross one of the minima and will decelerate rapidly as it reaches the local maximum at the origin, either falling back or crossing it. During this final phase, a significant peak in the curvature power spectrum can be generated. Our analysis reveals that this class of models produces more pronounced peaks than most quasi-inflection point scenarios with less tuning for the model parameters. Finally, we construct an explicit theoretically motivated inflationary scenario that is consistent with the latest CMB observations and capable of generating sufficiently large curvature perturbations for primordial black holes.

AB - We investigate the formation of large peaks in the inflationary curvature power spectrum from double-well potentials. In such scenarios, the initial CMB spectrum is created at large field values. Subsequently, the inflaton will cross one of the minima and will decelerate rapidly as it reaches the local maximum at the origin, either falling back or crossing it. During this final phase, a significant peak in the curvature power spectrum can be generated. Our analysis reveals that this class of models produces more pronounced peaks than most quasi-inflection point scenarios with less tuning for the model parameters. Finally, we construct an explicit theoretically motivated inflationary scenario that is consistent with the latest CMB observations and capable of generating sufficiently large curvature perturbations for primordial black holes.

KW - inflation

KW - primordial black holes

U2 - 10.1088/1475-7516/2023/09/002

DO - 10.1088/1475-7516/2023/09/002

M3 - Journal article

AN - SCOPUS:85171282444

VL - 2023

JO - Journal of Cosmology and Astroparticle Physics

JF - Journal of Cosmology and Astroparticle Physics

SN - 1475-7516

IS - 9

M1 - 002

ER -