Reconstruction of primordial power spectrum of curvature perturbation from the merger rate of primordial black hole binaries
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Publication:5026110
DOI10.1088/1475-7516/2021/04/031zbMath1485.83014arXiv2102.05280OpenAlexW3161211363MaRDI QIDQ5026110
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Publication date: 7 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2102.05280
Black holes (83C57) Quantum optics (81V80) Two-body problems (70F05) Perturbations in context of PDEs (35B20) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Gravitational waves (83C35)
Related Items (6)
Primordial black holes in peak theory with a non-Gaussian tail ⋮ Primordial black holes ensued from exponential potential and coupling parameter in nonminimal derivative inflation model ⋮ Galileon inflation evades the no-go for PBH formation in the single-field framework ⋮ Quantum loop effects on the power spectrum and constraints on primordial black holes ⋮ Constraints on the primordial curvature power spectrum by pulsar timing array data: a polynomial parameterization approach ⋮ Feasibility of primordial black hole Remnants as dark matter in view of Hawking radiation recoil
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