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Axions and other pseudoscalar fields comprise an interesting class of ultralight dark matter candidates, that may independently play a role in solving the strong $CP$ problem. In the presence of $CP$-violating sources, these pseudoscalar…

High Energy Physics - Phenomenology · Physics 2022-04-11 Shohei Okawa , Maxim Pospelov , Adam Ritz

We show that axion phenomenology may be significantly different than conventionally assumed in theories which exhibit late phase transitions (below the QCD scale). In such theories one can find multiple pseudoscalars with axion-like…

High Energy Physics - Phenomenology · Physics 2009-11-11 David B. Kaplan , Kathryn M. Zurek

A gauge invariant formulation for the massive axion is considered. The axion acquires mass through a topological term which couples a (pseudo)scalar and a third rank antisymmetric tensor. Duality, local and canonical equivalences with the…

High Energy Physics - Theory · Physics 2009-10-31 P. J. Arias , A. Khoudeir

The presence of axions introduces new diagrams at one-loop order to the two-photon decays of the neutral pion through axion-pion mixing. In this work, we calculate this correction, missing in all current calculations, in the framework of…

High Energy Physics - Phenomenology · Physics 2025-03-17 Zhen-Yan Lu , Yang Huang , Ji-Gui Cheng , Qi Lu , Shu-Peng Wang

In the context of string theory, axions appear to provide the most plausible solution of the strong CP problem. However, as has been known for a long time, in many string-based models, the axion coupling parameter F_a is several orders of…

High Energy Physics - Theory · Physics 2010-04-07 Peter Svrcek , Edward Witten

In this lecture we review several cosmological issues associated with the axion. Axion solves the strong CP problem and is a good candidate for the dark matter. Limits, which are imposed by the value of isocurvature fluctuations fraction in…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexey Anisimov

In the late 1970's, the axion was proposed as a solution to the Strong CP Problem, i.e. the puzzle why the strong interactions conserve parity P and the product CP of charge conjugation and parity in spite of the fact that the Standard…

High Energy Physics - Phenomenology · Physics 2021-02-24 Pierre Sikivie

We study the phenomenology of the 'companion-axion model' consisting of two coupled QCD axions. The second axion is required to rescue the Peccei-Quinn solution to the strong-CP problem from the effects of colored gravitational instantons.…

High Energy Physics - Phenomenology · Physics 2022-10-27 Zhe Chen , Archil Kobakhidze , Ciaran A. J. O'Hare , Zachary S. C. Picker , Giovanni Pierobon

We study the $\textit{complete}$ parameter space of a bulk axion in flat and warped extra spacetime dimensions. We characterize in detail the regimes where no single KK mode is produced along the canonical QCD axion line, and instead, it is…

High Energy Physics - Phenomenology · Physics 2025-04-14 Arturo de Giorgi , Maria Ramos

We study the cosmological evolution of the QCD axion coupled to hidden photons. For a moderately strong coupling, the motion of the axion field leads to an explosive production of hidden photons by tachyonic instability. We use lattice…

High Energy Physics - Phenomenology · Physics 2018-05-23 Naoya Kitajima , Toyokazu Sekiguchi , Fuminobu Takahashi

In supersymmetric theories, the Peccei-Quinn symmetry has a complex extension as a symmetry of the superpotential, so that the scalar potential always has an almost flat direction, the dilaton. We discuss how coherent oscillation of the…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Hashimoto , K. -I. Izawa , M. Yamaguchi , T. Yanagida

The axion mass receives a large correction from small instantons if the QCD gets strongly coupled at high energies. We discuss the size of the new CP violating phases caused by the fact that the small instantons are sensitive to the UV…

High Energy Physics - Phenomenology · Physics 2021-07-28 Ryuichiro Kitano , Wen Yin

We present a novel framework of the post-inflationary composite axion to address the strong CP problem without the cosmological domain wall problem. Conventional composite axion models lead to the domain wall number greater than one,…

High Energy Physics - Phenomenology · Physics 2026-04-30 Shihwen Hor , Yuichiro Nakai , Motoo Suzuki , Junxuan Xu

We use supersymmetric chiral dynamics perturbed by anomaly-mediated supersymmetry breaking to obtain a high-quality, composite axion that solves the strong CP problem. The strong dynamics arises from a supersymmetric SU(10) chiral gauge…

High Energy Physics - Phenomenology · Physics 2025-09-01 T. Gherghetta , H. Murayama , B. Noether , P. Quílez

It is firmly believed that the axion for solving the strong CP problem must come from the spontaneous breaking of an anomalous Peccei-Quinn global symmetry. Here we show a new possibility that the axion can be induced by a pseudo Goldstone…

High Energy Physics - Phenomenology · Physics 2023-07-11 Pei-Hong Gu

Inspired by recent studies of high-scale decay constant or flavorful QCD axions, we review and clarify their existence in effective string models with anomalous $U(1)$ gauge groups. We find that such models, when coupled to charged scalars…

High Energy Physics - Phenomenology · Physics 2019-01-21 Quentin Bonnefoy , Emilian Dudas

We consider the physical implications of very light axiodilatons motivated by a novel mechanism to substantially reduce the vacuum energy proposed in arXiv:2110.10352. We address the two main problems concerning the light axiodilaton that…

High Energy Physics - Phenomenology · Physics 2023-08-16 Philippe Brax , Cliff Burgess , Fernando Quevedo

The axion solution of the strong CP problem provides a number of possible windows to physics beyond the standard model, notably in the form of searches for solar axions and for galactic axion dark matter, but in a broader context also…

High Energy Physics - Phenomenology · Physics 2008-11-26 Georg G. Raffelt

We study cosmological solutions of (pseudo)scalar theories with periodic potentials, in the presence of arbitrary cosmological fluids -- including a cosmological constant of either sign. Independently of the initial misalignment angle and…

Cosmology and Nongalactic Astrophysics · Physics 2026-04-13 Gary Shiu , Flavio Tonioni , Hung V. Tran

In the Standard Model a Dark Matter candidate is missing, but it is relatively simple to enlarge the model including one or more suitable particles. We consider in this paper one such extension, inspired by simplicity and by the goal to…

High Energy Physics - Phenomenology · Physics 2022-10-05 Laura Covi , Sarif Khan