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A fast-rolling axion can transfer its kinetic energy to a gauge field via the Chern-Simons coupling, leading to copious production of gauge quanta, which can act as a source of gravitational waves (GWs) with potentially observable…

高能物理 - 唯象学 · 物理学 2025-10-21 Kai-Ge Zhang , Jian-Feng He , Chengjie Fu , Zong-Kuan Guo

Axion inflation entails a coupling of the inflaton field to gauge fields through the Chern-Simons term. This results in a strong gauge field production during inflation, which backreacts on the inflaton equation of motion. Here we show that…

宇宙学与河外天体物理 · 物理学 2020-08-13 Valerie Domcke , Veronica Guidetti , Yvette Welling , Alexander Westphal

We investigate the reheating process in an axion inflation model where the inflaton couples to non-Abelian gauge fields via the Chern-Simons coupling. The Chern-Simons coupling leads to the efficient production of gauge fields via a…

高能物理 - 唯象学 · 物理学 2025-03-04 Tomohiro Fujita , Kyohei Mukaida , Tenta Tsuji

Models of inflation based on axions, which owe their popularity to the robustness against UV corrections, have also a very distinct class of signatures. The relevant interactions of the axion are a non-perturbative oscillating contribution…

宇宙学与河外天体物理 · 物理学 2013-05-30 Neil Barnaby , Enrico Pajer , Marco Peloso

We numerically study axion-U(1) inflation, focusing on the regime where the coupling between axions and gauge fields results in significant backreaction from the amplified gauge fields during inflation. These amplified gauge fields not only…

宇宙学与河外天体物理 · 物理学 2025-05-28 Ramkishor Sharma , Axel Brandenburg , Kandaswamy Subramanian , Alexander Vikman

We consider a model of inflation in which the inflaton field is a rolling axion with a potential which is flat enough to support an intermediate phase of USR inflation. Because of the Chern-Simons interaction, one polarization of the gauge…

宇宙学与河外天体物理 · 物理学 2025-07-04 Alireza Talebian , Hassan Firouzjahi

We consider, in the context of axion-inflation, the \textit{Pure Natural Inflation} (PNI) model coupled with an SU(2) gauge sector via a Chern-Simons term. As the axion rolls down its potential, it dissipates energy in the gauge sector thus…

宇宙学与河外天体物理 · 物理学 2025-04-25 Ema Dimastrogiovanni , Matteo Fasiello , Alexandros Papageorgiou , Cristóbal Zenteno Gatica

We evaluate the quantum backreaction due to a gauge field coupled to a pseudo-scalar field driving a slow-roll inflationary stage, the so-called axion inflation. The backreaction is evaluated for the first time using a gauge invariant…

广义相对论与量子宇宙学 · 物理学 2024-10-23 Davide Campanella Galanti , Pietro Conzinu , Giovanni Marozzi , Simony Santos da Costa

In this paper, we examine the viability of inflation models with a spectator axion field coupled to both gravitational and SU(2) gauge fields via Chern-Simons couplings. Requiring phenomenological success of the axion-SU(2) sector…

广义相对论与量子宇宙学 · 物理学 2020-06-17 Leila Mirzagholi , Eiichiro Komatsu , Kaloian D. Lozanov , Yuki Watanabe

Previous studies demonstrate that the inflaton, when coupled to the hypercharge Chern-Simons density, can source an explosive production of helical hypermagnetic fields. Then, in the absence of fermion production, those fields have the…

高能物理 - 唯象学 · 物理学 2023-06-21 Yann Cado , Mariano Quirós

The coupling between a pseudo-scalar inflaton and a gauge field leads to an amount of additional density perturbations and gravitational waves (GWs) that is strongly sensitive to the inflaton speed. This naturally results in enhanced GWs at…

宇宙学与河外天体物理 · 物理学 2023-03-24 Juan Garcia-Bellido , Alexandros Papageorgiou , Marco Peloso , Lorenzo Sorbo

A fast-rolling axion can transfer its kinetic energy to gauge fields via the Chern-Simons coupling, leading to copious production of gauge quanta during inflation. The amplified gauge fields act as a source for both scalar and tensor…

高能物理 - 唯象学 · 物理学 2026-01-22 Kai-Ge Zhang , Jian-Feng He , Chengjie Fu , Zong-Kuan Guo

Models of axion inflation are particularly interesting since they provide a natural justification for the flatness of the potential over a super-Planckian distance, namely the approximate shift-symmetry of the inflaton. In addition, most of…

宇宙学与河外天体物理 · 物理学 2015-06-04 P. Daniel Meerburg , Enrico Pajer

The axionic inflaton with the Chern-Simons coupling may generate U(1) gauge fields and charged particles simultaneously. In order to incorporate the backreaction from the charged particles on the gauge fields, we develop a procedure to…

高能物理 - 唯象学 · 物理学 2022-09-14 Tomohiro Fujita , Jun'ya Kume , Kyohei Mukaida , Yuichiro Tada

In this work, we perform the first numerical study of strong scalar backreaction in spectator chromo-natural inflation (SCNI) in the case where the spectator sector decays during inflation. The tachyonic instability in scalar fluctuations,…

宇宙学与河外天体物理 · 物理学 2026-01-15 Mattia Cielo , Ema Dimastrogiovanni , Matteo Fasiello , Alexandros Papageorgiou

In this work, we study general features of a regime where gauge fields produced during inflation cause a strong backreaction on the background evolution and its impact on the spectrum and the correlation length of gauge fields. With this…

广义相对论与量子宇宙学 · 物理学 2023-11-08 R. Durrer , O. Sobol , S. Vilchinskii

Inflationary models equipped with Chern-Simons coupling between their axion and gauge sectors exhibit an array of interesting signals including a testable chiral gravitational wave spectrum. The energy injection in the gauge sector…

宇宙学与河外天体物理 · 物理学 2024-05-28 Ema Dimastrogiovanni , Matteo Fasiello , Martino Michelotti , Ogan Özsoy

Axion inflation, i.e. an axion-like inflaton coupled to an Abelian gauge field through a Chern-Simons interaction, comes with a rich and testable phenomenology. This is particularly true in the strong backreaction regime, where the gauge…

宇宙学与河外天体物理 · 物理学 2024-02-15 Valerie Domcke , Yohei Ema , Stefan Sandner

We perform an analytical study of the stability of the background solution of the model in which an inflaton, through an axionic coupling to a $U(1)$ gauge field, causes an amplification of the gauge field modes that strongly backreact on…

宇宙学与河外天体物理 · 物理学 2023-02-01 Marco Peloso , Lorenzo Sorbo

We study the non-linear dynamics of axion inflation, capturing for the first time the inhomogeneity and full dynamical range during strong backreaction, till the end of inflation. Accounting for inhomogeneous effects leads to a number of…

宇宙学与河外天体物理 · 物理学 2023-05-01 Daniel G. Figueroa , Joanes Lizarraga , Ander Urio , Jon Urrestilla
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