Built on

V. De Luca, G. Franciolini, A. Kehagias, M. Peloso, A. Riotto and C. Ünal, “The Ineludible non-Gaussianity of the Primordial Black Hole Abundance,” arXiv:1904.00970 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
D. H. Lyth, “The hybrid inflation waterfall and the primordial curvature perturbation,” JCAP 1205
Original
1904
Earlier work this paper cites.
B. J. Carr, Astrophys. J. 201, 1 (1975)
1975
Earlier work this paper cites.
M.Yu. Khlopov, A.G. Polnarev (Moscow, IPM). “Primordial black holes as a cosmological test of grand unification”, Phys.Lett.B97:383-387,1980 A.G.Polnarev, M.Yu.Khlopov “Primordial Black Holes and the ERA of Superheavy Particle Dominance in the Early Universe.” Astron. Zh. (1981), V. 58, PP. 706-715. [English translation: Sov. Astron. (1981) V. 25, P. 406]
1981
Earlier work this paper cites.
A. A. Starobinsky and J. Yokoyama, “Equilibrium state of a selfinteracting scalar field in the De Sitter background,” Phys. Rev. D 50
1986
Earlier work this paper cites.
D. Babich, P. Creminelli and M. Zaldarriaga, “The Shape of non-Gaussianities,” JCAP 0408
2004
Earlier work this paper cites.
J. R. Bond, S. Cole, G. Efstathiou and N. Kaiser, “Excursion set mass functions for hierarchical Gaussian fluctuations,” Astrophys. J. 379
2007
Earlier work this paper cites.
J. R. Bond, A. V. Frolov, Z. Huang and L. Kofman, “Non-Gaussian Spikes from Chaotic Billiards in Inflation Preheating,” Phys. Rev. Lett. 103
Original
2009
Earlier work this paper cites.

Similar

B. Carr and J. Silk, “Primordial Black Holes as Generators of Cosmic Structures,” doi:10.1093/mnras/sty1204 arXiv:1801.00672 [astro-ph.CO]; S. Clesse and J. García-Bellido, “Seven Hints for Primordial Black Hole Dark Matter,” arXiv:1711.10458 [astro-ph.CO]; B. J. Carr, K. Kohri, Y. Sendouda and J. Yokoyama, “New cosmological constraints on primordial black holes,” Phys. Rev. D 81
Original
2010
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B. J. Carr, K. Kohri, Y. Sendouda and J. Yokoyama, “New cosmological constraints on primordial black holes,” Phys. Rev. D 81
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M. Kopp, S. Hofmann and J. Weller, “Separate Universes Do Not Constrain Primordial Black Hole Formation,” Phys. Rev. D 83
Original
2011
Cited alongside, same era.
V. Demozzi, A. Linde and V. Mukhanov, “Supercurvaton,” JCAP 1104
Original
2011
Cited alongside, same era.

Then

X. Dong, B. Horn, E. Silverstein and A. Westphal, “Simple exercises to flatten your potential,” Phys. Rev. D 84
Original
2014
Later among the works it cites.
R. Kallosh, A. Linde and D. Roest, “Large field inflation and double α \alpha -attractors,” JHEP 1408
Original
2014
Later among the works it cites.
R. Kallosh and A. Linde, “Escher in the Sky,” Comptes Rendus Physique 16
Original
2015
Later among the works it cites.
T. Nakama, B. Carr and J. Silk, “Limits on primordial black holes from μ \mu distortions in cosmic microwave background,” Phys. Rev. D 97
Original
2016
Later among the works it cites.
B. Carr, M. Raidal, T. Tenkanen, V. Vaskonen and H. Veermäe, “Primordial black hole constraints for extended mass functions,” Phys. Rev. D 96

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2019

Primordial Black Holes from non-Gaussian tails

Panagopoulos, George, Silverstein, Eva

Understand

We develop a primordial black hole (PBH) production mechanism, deriving non-Gaussian tails from interacting quantum fields during early universe inflation.

The multi-field potential landscape may contain relatively flat directions, as a result of energetically favorable adjustments of fields coupled to the inflaton.
Such additional fields do not contribute to CMB fluctuations given a sufficient large-scale decay, related to a gap in the critical exponents computed using stochastic methods.
Along such directions transverse to the inflaton, the field makes rare jumps to large values.

Built on

V. De Luca, G. Franciolini, A. Kehagias, M. Peloso, A. Riotto and C. Ünal, “The Ineludible non-Gaussianity of the Primordial Black Hole Abundance,” arXiv:1904.00970 [astro-ph.CO]
Original
1904
Earlier work this paper cites.
D. H. Lyth, “The hybrid inflation waterfall and the primordial curvature perturbation,” JCAP 1205
Original
1904
Earlier work this paper cites.
B. J. Carr, Astrophys. J. 201, 1 (1975)
1975
Earlier work this paper cites.
M.Yu. Khlopov, A.G. Polnarev (Moscow, IPM). “Primordial black holes as a cosmological test of grand unification”, Phys.Lett.B97:383-387,1980 A.G.Polnarev, M.Yu.Khlopov “Primordial Black Holes and the ERA of Superheavy Particle Dominance in the Early Universe.” Astron. Zh. (1981), V. 58, PP. 706-715. [English translation: Sov. Astron. (1981) V. 25, P. 406]
1981
Earlier work this paper cites.
A. A. Starobinsky and J. Yokoyama, “Equilibrium state of a selfinteracting scalar field in the De Sitter background,” Phys. Rev. D 50
1986
Earlier work this paper cites.
D. Babich, P. Creminelli and M. Zaldarriaga, “The Shape of non-Gaussianities,” JCAP 0408
2004
Earlier work this paper cites.
J. R. Bond, S. Cole, G. Efstathiou and N. Kaiser, “Excursion set mass functions for hierarchical Gaussian fluctuations,” Astrophys. J. 379
2007
Earlier work this paper cites.
J. R. Bond, A. V. Frolov, Z. Huang and L. Kofman, “Non-Gaussian Spikes from Chaotic Billiards in Inflation Preheating,” Phys. Rev. Lett. 103
Original
2009
Earlier work this paper cites.