Axion inflation in the strong-backreaction regime: decay of the Anber-Sorbo solution
arXiv:2309.04254 · doi:10.1007/JHEP11(2023)183
Abstract
Axion inflation coupled to Abelian gauge fields via a Chern-Simons-like term of the form represents an attractive inflationary model with a rich phenomenology, including the production of magnetic fields, black holes, gravitational waves, and the matter-antimatter asymmetry. In this work, we focus on a particular regime of axion inflation, the so-called Anber-Sorbo (AS) solution, in which the energy loss in the gauge-field production provides the dominant source of friction for the inflaton motion. We revisit the AS solution and confirm that it is unstable. Contrary to earlier numerical works that attempted to reach the AS solution starting from a regime of weak backreaction, we perform, for the first time, a numerical evolution starting directly from the regime of strong backreaction. Our analysis strongly suggests that, at least as long as one neglects spatial inhomogeneities in the inflaton field, the AS solution has no basin of attraction, not even a very small one that might have been missed in previous numerical studies. Our analysis employs an arsenal of analytical and numerical techniques, some established and some newly introduced, including (1) linear perturbation theory along the lines of arXiv:2209.08131, (2) the gradient expansion formalism (GEF) developed in arXiv:2109.01651, (3) a new linearized version of the GEF, and (4) the standard mode-by-mode approach in momentum space in combination with input from the GEF. All these methods yield consistent results confirming the instability of the AS solution, which renders the dynamics of axion inflation in the strong-backreaction regime even more interesting than previously believed.
40 pages, 11 figures
References in corpus (11)
- The Swampland: Introduction and Review
- Large Nongaussianity in Axion Inflation
- Gravitational Wave signatures of inflationary models from Primordial Black Hole Dark Matter
- Gravitational waves at interferometer scales and primordial black holes in axion inflation
- Primordial Gravitational Waves from Axion-Gauge Fields Dynamics
- Inflation and Primordial Black Holes
- Lattice Simulations of Axion-U(1) Inflation
- Dissipative Axial Inflation
- Instability in axion inflation with strong backreaction from gauge modes
- Backreaction from gauge fields produced during inflation
- Numerical study of the Schwinger effect in axion inflation
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- On the Schwinger effect during axion inflation
- On Sphaleron Heating in the Presence of Fermions
- Magnetogenesis from axion-SU(2) inflation
- Primordial Power Spectrum and Bispectrum from Lattice Simulations of Axion-U(1) Inflation
- Strong backreaction of gauge quanta produced during inflation
- Gravitational waves from axion inflation in the gradient expansion formalism. Part I. Pure axion inflation
- On the prospects of thermalization of axion-SU(2) inflation
- Gravitational Waves from a Gauge Field Non-minimally Coupled to Gravity
- Gravitational waves from axion inflation in the gradient expansion formalism. Part II. Fermionic axion inflation
- Perturbative limits on axion-SU(2) gauge dynamics during inflation from the energy density of spin-2 particles
- Stringy constraints on primordial electromagnetic fields in axion inflation
- Vector dark matter production during inflation in the gradient-expansion formalism
- Gravitational Waves from Gauge Quanta Produced during Inflation