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The QCD axion cosmology depends crucially on whether the QCD axion is present during inflation or not. We point out that contrary to the standard criterion, the Peccei-Quinn (PQ) symmetry could remain unbroken during inflation, even when…

高能物理 - 唯象学 · 物理学 2023-06-14 Yunjia Bao , JiJi Fan , Lingfeng Li

We argue that the QCD axion can arise from many aligned axions with decay constants much smaller than the conventional axion window. If the typical decay constant is of {\cal O}{(100)} GeV to 1 TeV, one or more of the axions or saxions may…

高能物理 - 唯象学 · 物理学 2016-02-03 Tetsutaro Higaki , Kwang Sik Jeong , Naoya Kitajima , Fuminobu Takahashi

Murayama proposed a GeV-scale axion theory where the up-quark mass term is generated dynamically by the QCD chiral condensate, spontaneously breaking a Peccei-Quinn symmetry. It predicts a too large mass splitting between neutral and…

高能物理 - 唯象学 · 物理学 2026-02-25 Luca Di Luzio , Michele Redi , Alessandro Strumia , Andrea Tesi , Arsenii V. Titov

Axion rotations can simultaneously explain the dark matter abundance and the baryon asymmetry of the Universe by kinetic misalignment and axiogenesis. We consider a scenario in which the Peccei-Quinn symmetry breaking field is as large as…

高能物理 - 唯象学 · 物理学 2024-09-25 Raymond T. Co , Masaki Yamada

Experimental limits on the violation of four-dimensional Lorentz invariance imply that noncommutativity among ordinary spacetime dimensions must be small. Noncommutativity among extra, compactified spatial dimensions, however, is far less…

高能物理 - 唯象学 · 物理学 2009-11-07 Carl E. Carlson , Christopher D. Carone

Axions are some of the best motivated particles beyond the Standard Model. We show how the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from $10^{-22}$ eV to $10^7$ GeV, can lead to nongravitational…

宇宙学与河外天体物理 · 物理学 2020-04-15 Asimina Arvanitaki , Savas Dimopoulos , Marios Galanis , Luis Lehner , Jedidiah O. Thompson , Ken Van Tilburg

We investigate the cosmology of an axion that is fundamentally non-compact. During inflation, fluctuations of the effectively massless field populate many QCD vacua, thereby evading conventional isocurvature constraints while generating…

高能物理 - 唯象学 · 物理学 2025-12-24 Georgios K. Karananas , Mikhail Shaposhnikov , Sebastian Zell

We study the QCD axion arising from the 5th component of a bulk $U(1)$ gauge field in a five-dimensional warped grand unified theory, and determine the viable range of the axion decay constant $f_a$. Unlike flat extra dimensions, where…

高能物理 - 唯象学 · 物理学 2025-12-18 Gongjun Choi , Tony Gherghetta

In presence of a magnetic field, photons can mix with any particle having a two-photon vertex. In theories with large compact extra-dimensions, there exists a hierachy of massive Kaluza-Klein gravitons that couple to any photon entering a…

高能物理 - 唯象学 · 物理学 2009-10-07 Cedric Deffayet , Jean-Philippe Uzan

Axion cosmology is reexamined taking into account effect of kinetic pseudo Nambu-Goldstone modes, with its importance recently pointed out. When Peccei-Quinn (PQ) symmetry is broken by a chiral U(1) singlet, it is found that the effect of…

高能物理 - 唯象学 · 物理学 2022-06-01 Motohiko Yoshimura

We show that in any invisible axion model due to the effects of effective non-renormalizable interactions related to an energy scale near the Peccei-Quinn, grand unification or even the Planck scale, active neutrinos necessarily acquire…

高能物理 - 唯象学 · 物理学 2009-11-11 Alex G. Dias , V. Pleitez

Axions are hypothetical pseudoscalar particles introduced initially as a solution to the Strong CP problem in Quantum Chromodynamics (QCD), and they also arise naturally in a broad class of low-energy compactifications of string theory.…

高能物理 - 唯象学 · 物理学 2025-12-24 Amedeo M. Favitta

A QCD axion with a time-dependent decay constant has been known to be able to accommodate high-scale inflation without producing topological defects or too large isocurvature perturbations on CMB scales. We point out that a dynamical decay…

高能物理 - 唯象学 · 物理学 2016-08-29 Takeshi Kobayashi , Fuminobu Takahashi

We investigate the axion quality problem in warped extra-dimensional models in which the QCD axion arises as the Wilson-line mode of a five-dimensional $U(1)$ gauge field compactified on an $S^1/\mathbb{Z}_2$ orbifold. Higher-dimensional…

高能物理 - 唯象学 · 物理学 2026-05-29 Kiwoon Choi , Chang Hyeon Lee , Chang Sub Shin

It was shown that the required high quality of the Peccei-Quinn (PQ) symmetry can be a natural outcome of the multiple QCD axions model. In the axiverse, a hypothetical mass mixing between the QCD axions and axion-like particles (ALPs) can…

高能物理 - 唯象学 · 物理学 2024-08-29 Hai-Jun Li

In the framework where the strong coupling is dynamical, the QCD sector may confine at a much higher temperature than it would in the Standard Model, and the temperature-dependent mass of the QCD axion evolves in a non-trivial way. We find…

高能物理 - 唯象学 · 物理学 2022-01-12 Lucien Heurtier , Fei Huang , Tim M. P. Tait

We revisit the domain wall problem for QCD axion models with more than one quark charged under the Peccei-Quinn symmetry. Symmetry breaking during or after inflation results in the formation of a domain wall network which would cause cosmic…

高能物理 - 唯象学 · 物理学 2023-07-11 Konstantin A. Beyer , Subir Sarkar

Composite axion scenarios offer a robust field theoretic justification for the existence of a Peccei-Quinn symmetry of high quality. We present a new class of realizations that are naturally embedded in Grand-Unified Theories, retain…

高能物理 - 唯象学 · 物理学 2021-11-10 Luca Vecchi

The QCD axion and axion-like particles, as leading dark matter candidates, can also have interesting implications for dark matter substructures if the Peccei-Quinn symmetry is broken after inflation. In such a scenario, axion perturbations…

高能物理 - 唯象学 · 物理学 2024-09-20 Jae Hyeok Chang , Patrick J. Fox , Huangyu Xiao

We present global fits of cosmologically stable axion-like particle and QCD axion models in the mass range 0.1 neV to 10 eV. We focus on the case where the Peccei-Quinn symmetry is broken before the end of inflation, such that the initial…

高能物理 - 唯象学 · 物理学 2020-08-19 Sebastian Hoof , Felix Kahlhoefer , Pat Scott , Christoph Weniger , Martin White