Constant-rate inflation: primordial black holes from conformal weight transitions

A bstract Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes with a significant deviation from the standard slow-roll conditions at both the growing and decaying phases of the power spectrum. We derive an...

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Published inThe journal of high energy physics Vol. 2021; no. 11; pp. 1 - 26
Main Authors Ng, Kin-Wang, Wu, Yi-Peng
Format Journal Article
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 11.11.2021
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Abstract A bstract Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes with a significant deviation from the standard slow-roll conditions at both the growing and decaying phases of the power spectrum. We derive analytic solutions for the curvature perturbations with respect to the late-time scaling dimensions (conformal weights) constrained by the dilatation symmetry of the de Sitter background and show that the continuity of conformal weights across different rolling phases is protected by the adiabatic condition of the inflaton perturbation. The temporal excitation of subleading states (with the next-to-lowest conformal weights), recorded as the “steepest growth” of the power spectrum, is triggered by the entropy production in the transition from the slow-roll to the constant-rate phases.
AbstractList Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes with a significant deviation from the standard slow-roll conditions at both the growing and decaying phases of the power spectrum. We derive analytic solutions for the curvature perturbations with respect to the late-time scaling dimensions (conformal weights) constrained by the dilatation symmetry of the de Sitter background and show that the continuity of conformal weights across different rolling phases is protected by the adiabatic condition of the inflaton perturbation. The temporal excitation of subleading states (with the next-to-lowest conformal weights), recorded as the “steepest growth” of the power spectrum, is triggered by the entropy production in the transition from the slow-roll to the constant-rate phases.
A bstract Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes with a significant deviation from the standard slow-roll conditions at both the growing and decaying phases of the power spectrum. We derive analytic solutions for the curvature perturbations with respect to the late-time scaling dimensions (conformal weights) constrained by the dilatation symmetry of the de Sitter background and show that the continuity of conformal weights across different rolling phases is protected by the adiabatic condition of the inflaton perturbation. The temporal excitation of subleading states (with the next-to-lowest conformal weights), recorded as the “steepest growth” of the power spectrum, is triggered by the entropy production in the transition from the slow-roll to the constant-rate phases.
Abstract Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes with a significant deviation from the standard slow-roll conditions at both the growing and decaying phases of the power spectrum. We derive analytic solutions for the curvature perturbations with respect to the late-time scaling dimensions (conformal weights) constrained by the dilatation symmetry of the de Sitter background and show that the continuity of conformal weights across different rolling phases is protected by the adiabatic condition of the inflaton perturbation. The temporal excitation of subleading states (with the next-to-lowest conformal weights), recorded as the “steepest growth” of the power spectrum, is triggered by the entropy production in the transition from the slow-roll to the constant-rate phases.
ArticleNumber 76
Author Wu, Yi-Peng
Ng, Kin-Wang
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  surname: Ng
  fullname: Ng, Kin-Wang
  organization: Institute of Physics, Academia Sinica, Institute of Astronomy and Astrophysics, Academia Sinica
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  email: ywu@lpthe.jussieu.fr
  organization: Laboratoire de Physique Théorique et Hautes Energies (LPTHE), UMR 7589 CNRS & Sorbonne Université
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Issue 11
Keywords Conformal Field Theory
Space-Time Symmetries
Cosmology of Theories beyond the SM
power spectrum
symmetry: de Sitter
black hole: formation
critical phenomena
invariance: scale
horizon: crossing
inflaton: potential
field theory: conformal
black hole: primordial
scaling: dimension
boundary condition
vacuum state
space-time: de Sitter
symmetry: dilation
inflation: model
field theory: scalar: massless
Hubble constant
curvature: perturbation
background: de Sitter
dark matter
correlation function
non-Gaussianity
slow-roll approximation: violation
Language English
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Snippet A bstract Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes...
Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes with a...
Abstract Constant-rate inflation, including ultra-slow-roll inflation as a special case, has been widely applied to the formation of primordial black holes...
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SubjectTerms Adiabatic conditions
Astrophysics
Black holes
Classical and Quantum Gravitation
Conformal Field Theory
Cosmology of Theories beyond the SM
Elementary Particles
Exact solutions
Gravitational waves
High energy physics
High Energy Physics - Phenomenology
High Energy Physics - Theory
Mathematical analysis
Perturbation
Phases
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Quantum Physics
Regular Article - Theoretical Physics
Relativity Theory
Space-Time Symmetries
Spacetime
String Theory
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Title Constant-rate inflation: primordial black holes from conformal weight transitions
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