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Drew Jamieson ^1,*, Angelo Caravano ^2,†, and Eiichiro Komatsu ^1,3,4

¹Max-Planck-Institut für Astrophysik, Karl-Schwarzschild-Straße 1, 85748 Garching, Germany
²Institut d’Astrophysique de Paris, UMR 7095 du CNRS et de Sorbonne Université, 98 bis Bd Arago, 75014 Paris, France
³Ludwig-Maximilians-Universität München, Schellingstr. 4, 80799 München, Germany
⁴Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), Todai Institutes for Advanced Study, The University of Tokyo, Kashiwa 277-8583, Japan

^*Contact author: jamieson@mpa-garching.mpg.de
^†Contact author: caravano@iap.fr

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Articles Citing

Primordial power spectrum and bispectrum from lattice simulations of axion-U(1) inflation

Suppression of scalar perturbations due to a heavy axion

Parity-odd four-point correlation function from the DESI data release 1 luminous red galaxy sample

Nonlinear physics of axion inflation

Gravitational waves from axion inflation in the gradient expansion formalism. Part I. Pure axion inflation

Axion inflation in the regime of homogeneous backreaction

Classical equipartition dynamics between axions and non-Abelian gauge fields

Perturbative limits on axion-SU(2) gauge dynamics during inflation from the energy density of spin-2 particles

Revisiting primordial black hole dark matter from axion inflation

Nonlinear lattice framework for inflation: Bridging stochastic inflation and the δN formalism

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