Cosmological implications of \(n_s \approx 1\) in light of the Hubble tension

DOI10.1016/j.physletb.2022.137143zbMath1497.85009arXiv2112.06710OpenAlexW4229076386MaRDI QIDQ2672807

Fuminobu Takahashi, Wen Yin

Publication date: 13 June 2022

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2112.06710

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Other elementary particle theory in quantum theory (81V25) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Galactic and stellar structure (85A15)

Related Items (2)

Inflationary potential as seen from different angles: model compatibility from multiple CMB missions ⋮ Tracking the multifield dynamics with cosmological data: a Monte Carlo approach

Cites Work

• Multi-natural inflation in supergravity
• Axion models with high scale inflation
• An \(M\) theory solution to the strong CP-problem, and constraints on the axiverse
• Elliptic inflation: interpolating from natural inflation to \(R^{2}\)-inflation
• The type IIB string axiverse and its low-energy phenomenology
• Dark matter in axion landscape
• Inflation from periodic extra dimensions
• Kilobyte Cosmic Birefringence from ALP domain walls
• Superradiance in string theory
• Stochastic axion dark matter in axion landscape
• A general proof of the conservation of the curvature perturbation
• Effects of cosmological moduli fields on cosmic microwave background
• Generating the curvature perturbation without an inflaton

This page was built for publication: Cosmological implications of \(n_s \approx 1\) in light of the Hubble tension