Scaling behavior of observables as a model characteristic in multifield inflation

DOI10.1088/1475-7516/2023/04/039zbMath1522.83303arXiv2212.09830OpenAlexW4365451765MaRDI QIDQ6040466

Monika Lynker, Rolf Schimmrigk

Publication date: 17 May 2023

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2212.09830

zbMATH Keywords

inflationcosmology of theories beyond the SMphysics of the early universeinflation and CMBR theory

Mathematics Subject Classification ID

Unified quantum theories (81V22) Geometrodynamics and the holographic principle (83E05) Gravitational energy and conservation laws; groups of motions (83C40) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Difference equations, scaling ((q)-differences) (39A13) Effectivity, complexity and computational aspects of algebraic geometry (14Q20) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)

Cites Work

• Unnamed Item
• Automorphic inflation
• Generalized two-field \(\alpha\)-attractor models from the hyperbolic triply-punctured sphere
• A general framework of automorphic inflation
• Modular inflation observables and \(j\)-inflation phenomenology
• Generalized two-field \(\alpha\)-attractor models from geometrically finite hyperbolic surfaces
• The infrared behavior of tame two-field cosmological models
• Hidden symmetries of two-field cosmological models
• A new type of isotropic cosmological models without singularity
• Inflation in multi-field modified DBM potentials
• Modular inflation at higher levelN
• Multi-field inflation in high-slope potentials
• Inflation and String Theory
• Hyperbolic field space and swampland conjecture for DBI scalar