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相关论文: The Flavor of QCD Axion Dark Matter

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Standard Model extensions with light axions are well-motivated by the observed Dark Matter abundance and the Peccei-Quinn solution to the Strong CP Problem. In general such axions can have large flavor-violating couplings to SM fermions,…

高能物理 - 唯象学 · 物理学 2023-03-24 Robert Ziegler

Axion models with generation-dependent Peccei-Quinn charges can lead to flavor-changing neutral currents, thus motivating QCD axion searches at precision flavor experiments. We rigorously derive limits on the most general effective…

高能物理 - 唯象学 · 物理学 2020-08-05 Jorge Martin Camalich , Maxim Pospelov , Pham Ngoc Hoa Vuong , Robert Ziegler , Jure Zupan

Precision flavor experiments can look for the QCD axion complementarily to usual searches with axion helio- and haloscopes, allowing to test PQ breaking scales as high as $10^{12} \, {\rm GeV}$. Such searches are sensitive to…

高能物理 - 唯象学 · 物理学 2019-05-06 Robert Ziegler

We propose simple scenarios where lepton flavor-violating couplings generate the observed dark matter abundance through freeze-in of an axion-like particle with mass in the few keV range. Compared to flavor-diagonal freeze-in, this…

高能物理 - 唯象学 · 物理学 2023-05-03 Paolo Panci , Diego Redigolo , Thomas Schwetz , Robert Ziegler

The QCD axion is one of the best motivated dark matter candidates. The misalignment mechanism is well known to produce an abundance of the QCD axion consistent with dark matter for an axion decay constant of order $10^{12}$ GeV. For a…

高能物理 - 唯象学 · 物理学 2020-11-02 Junwu Huang , Amalia Madden , Davide Racco , Mario Reig

We discuss a QCD-scale composite axion model arising from dark QCD coupled to QCD. The presently proposed scenario not only solves the strong CP problem, but also is compatible with the preheating setup for the QCD baryogenesis. The…

高能物理 - 唯象学 · 物理学 2024-09-26 Bin Wang , Shinya Matsuzaki , Hiroyuki Ishida

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

Proposed half a century ago, the quantum chromodynamics (QCD) axion explains the lack of charge and parity violation in the strong interactions and is a compelling candidate for cold dark matter. The last decade has seen the rapid…

高能物理 - 实验 · 物理学 2025-04-16 Masha Baryakhtar , Leslie Rosenberg , Gray Rybka

It is difficult to construct a post-inflation QCD axion model that solves the axion quality problem (and hence the Strong CP problem) without introducing a cosmological disaster. In a post-inflation axion model, the axion field value is…

高能物理 - 唯象学 · 物理学 2024-08-27 Qianshu Lu , Matthew Reece , Zhiquan Sun

Axion dark matter coupled via QCD induces a non-zero differential acceleration between test masses of different composition. Tests of the equivalence principle, like the recent MICROSCOPE space mission, are sensitive to such a signal. We…

高能物理 - 唯象学 · 物理学 2025-04-02 Jordan Gué , Peter Wolf , Aurélien Hees

The QCD axion is a well-motivated hypothetical particle beyond the Standard Model (SM) and a compelling dark matter candidate. Its relic abundance is highly sensitive to the thermal history of the universe when the temperature is around the…

高能物理 - 唯象学 · 物理学 2025-06-26 Kun-Feng Lyu , Yue Zhao

We investigate the complementary information to be gained from inflationary gravitational wave (IGW) signals and searches for QCD axion dark matter. We focus on post-inflationary Peccei-Quinn (PQ) breaking axion models that are…

宇宙学与河外天体物理 · 物理学 2026-01-09 Andrew Cheek , Anish Ghoshal , Debarun Paul

The axion-like particle (ALP) is a well-motivated extension of the Standard Model. In this work, we revisit the sensitivity of forward accelerator experiments to light long-lived ALPs, and analyze flavor constraints. Our analysis…

高能物理 - 唯象学 · 物理学 2025-12-05 Tong Li , Michael A. Schmidt , Man Yuan

The axion is a hypothetical elementary particle postulated by the Peccei-Quinn theory to resolve the strong CP problem in QCD. If axions exist and have low mass, they are a candidate for dark matter as well. So far our knowledge of the…

高能物理 - 格点 · 物理学 2019-03-26 Y. Nakamura , G. Schierholz

It is shown that the post-inflationary quantum chromodynamics (QCD) axion need not lead to a unique one-parameter prediction for the dark matter abundance whenever small explicit Peccei-Quinn symmetry breaking becomes dynamically relevant…

高能物理 - 唯象学 · 物理学 2026-05-21 Michael Zantedeschi

The dark sector offers a compelling theoretical framework for addressing the nature of dark matter while potentially solving other fundamental problems in physics. This review focuses on light dark flavored sector models, which are those…

高能物理 - 唯象学 · 物理学 2025-03-24 Jorge Martin Camalich , Robert Ziegler

The Axion is a particle arising from the Peccei-Quinn solution to the strong CP problem. Peccei-Quinn symmetry breaking in the early universe could produce a large number of axions which would still be present today, making the axion a…

宇宙学与河外天体物理 · 物理学 2011-12-07 Dmitry Lyapustin

We investigate the properties of QCD axion at low temperature and moderate density in the Nambu-Jona-Lasinio model with instanton induced interactions by simultaneously considering the scalar and pseudo-scalar condensates in both…

高能物理 - 唯象学 · 物理学 2025-01-22 Zhao Zhang , Wenhao Zhao

Preferred axion models are minimal realizations of the Peccei-Quinn solution to the strong CP problem while providing a dark matter candidate. These models invoke new heavy quarks that interact strongly with the Standard Model bringing them…

高能物理 - 唯象学 · 物理学 2025-03-26 Andrew Cheek , Ui Min

Many existing and proposed experiments targeting QCD axion dark matter (DM) can also search for a broad class of axion-like particles (ALPs). We analyze the experimental sensitivities to electromagnetically-coupled ALP DM in different…

高能物理 - 唯象学 · 物理学 2019-08-07 Nikita Blinov , Matthew J. Dolan , Patrick Draper , Jonathan Kozaczuk
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