Note on the bispectrum and one-loop corrections in single-field inflation with primordial black hole formation

Abstract

Primordial black holes can be formed from the collapse of large-amplitude perturbation on small scales in the early Universe. Such an enhanced spectrum can be realized by introducing a flat region in the potential of single-field inflation, which makes the inflaton go into a temporary ultraslow-roll period. In this paper, we calculate the bispectrum of curvature perturbation in such a scenario. We explicitly confirm that bispectrum satisfies Maldacena's theorem. At the end of the ultraslow-roll period, the bispectrum is generated by bulk interaction and field redefinition. At the end of inflation, bispectrum is generated only by bulk interaction. We also calculate the one-loop correction to the power spectrum from the bispectrum, called the source method. We find it consistent with the calculation of the one-loop correction from the second-order expansion of in-in perturbation theory.

Accepted Physical Review D. Response to criticism can be read from previous versions. arXiv admin note: text overlap with arXiv:2211.03395

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Cited by in corpus (30)

• Constraining Primordial Black Hole Formation from Single-Field Inflation
• No-go for the formation of heavy mass Primordial Black Holes in Single Field Inflation
• One loop to rule them all: Perturbativity in the presence of ultra slow-roll dynamics
• Realisation of the ultra-slow roll phase in Galileon inflation and PBH overproduction
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• Large fluctuations and Primordial Black Holes
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