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相关论文: Cosmic Axion Spin Precession Experiment (CASPEr)

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Axion-like particles are dark matter candidates motivated by the Peccei-Quinn mechanism and also occur in effective field theories where their masses and photon couplings are independent. We estimate the dispersion of circularly polarized…

宇宙学与河外天体物理 · 物理学 2019-08-13 Günter Sigl , Pranjal Trivedi

We review the physics of ultralight axion-like particles (ALPs) as dark matter candidates and the experimental strategies used to search for them with precision and quantum technologies. In the ultralight regime, the enormous occupation…

高能物理 - 唯象学 · 物理学 2026-03-25 Sreemanti Chakraborti

We report on the search for a new spin-dependent P- and T-violating interaction between nucleons mediated by light, pseudoscalar bosons such as the axion which was invented to solve the strong CP problem. Our experimental approach is to use…

We show that dark matter axions or axion-like particles (ALP) induce spontaneously alternating electric currents in conductors along the external magnetic fields due to the (medium) axial anomaly, realizing the chiral magnetic effects…

高能物理 - 唯象学 · 物理学 2024-09-05 Deog Ki Hong , Sang Hui Im , Kwang Sik Jeong , Dong-han Yeom

We present a search for axion-like polarization oscillations in the cosmic microwave background (CMB) with observations from the Keck Array. A local axion field induces an all-sky, temporally sinusoidal rotation of CMB polarization. A CMB…

Axions or more generally axion-like particles (ALPs) are pseudo-scalar particles predicted by many extensions of the Standard Model of particle physics (SM) and considered as viable candidates for dark matter (DM) in the universe. If they…

高能天体物理现象 · 物理学 2020-05-20 Ahmed Ayad , Geoff Beck

Axions, originally proposed to solve the strong CP problem of quantum chromodynamics, emerge now as leading candidates of WISP dark matter. The rich phenomenology associated to the light and stable QCD axion can be described as an effective…

We propose using the storage ring EDM method to search for the axion dark matter induced EDM oscillation in nucleons. The method uses a combination of B and E-fields to produce a resonance between the $g-2$ spin precession frequency and the…

高能物理 - 实验 · 物理学 2019-04-17 Seung Pyo Chang , Selcuk Haciomeroglu , On Kim , Soohyung Lee , Seongtae Park , Yannis K. Semertzidis

The search for axions and axion-like particles (ALPs) remains a major endeavor in modern physics investigation. Axions play essential roles in the quest to understand dark matter, the strong CP problem, and various astrophysical phenomena.…

高能物理 - 唯象学 · 物理学 2024-12-13 Maurizio Giannotti

Axions and axion-like particles (ALPs) arise naturally in many extensions of the Standard Model and are among the well-motivated candidates for dark matter. In the presence of magnetic fields of galaxy clusters, Cosmic Microwave Background…

宇宙学与河外天体物理 · 物理学 2026-03-11 Harsh Mehta , Anaya Dixit , Suvodip Mukherjee , Joseph Silk

We explore whether the axion which solves the strong CP problem can naturally be much lighter than the canonical QCD axion. The $Z_\mathcal{N}$ symmetry proposed by Hook, with $\mathcal{N}$ mirror and degenerate worlds coexisting in Nature…

高能物理 - 唯象学 · 物理学 2021-11-09 Pablo Quilez , Luca Di Luzio , Belen Gavela , Andreas Ringwald

Cosmological axions/axion-like particles can compose a significant part of dark matter; however, the uncertainty of their mass is large. Here, we propose to search the axions using a cylindrical capacitor, in which the static electric field…

高能物理 - 唯象学 · 物理学 2024-06-21 Wenming Chen , Yu Gao , Qiaoli Yang

The SUPerconduction AXion search experiment (Supax) is a future haloscope-type detector designed to probe axion-like particles (ALPs) as candidates for dark matter and solutions to the strong-CP problem in the mass range between $8\,\mu$eV…

Axion-like particles (ALPs) provide a promising direction in the search for new physics, while a wide range of models incorporate ALPs. We point out that future neutrino experiments, such as DUNE, possess competitive sensitivity to ALP…

高能物理 - 唯象学 · 物理学 2021-05-19 Vedran Brdar , Bhaskar Dutta , Wooyoung Jang , Doojin Kim , Ian M. Shoemaker , Zahra Tabrizi , Adrian Thompson , Jaehoon Yu

We study an axion-like particle (ALP) that experiences the first-order phase transition with respect to its mass or potential minimum. This can be realized if the ALP obtains a potential from non-perturbative effects of SU($N$) gauge theory…

高能物理 - 唯象学 · 物理学 2023-04-05 Shota Nakagawa , Fuminobu Takahashi , Masaki Yamada , Wen Yin

Axion-like particles (ALPs), the QCD axion, and dark photons in the MeV-GeV mass range are motivated by various dark matter models and the strong CP problem, and are ubiquitous in extensions of the Standard Model. A long-standing blind spot…

高能物理 - 唯象学 · 物理学 2026-04-20 Sarah Gaiser , Alessandro Russo , Philip Schuster

Weakly interactive slim particles (WISPs), including the QCD axion, axion-like particles (ALPs), and hidden photons, are considered to be strong candidates for the dark matter carrier particle. The microwave cavity experiment WISPDMX is the…

仪器与探测器 · 物理学 2015-11-11 Le Hoang Nguyen , Dieter Horns , Andrei Lobanov , Andreas Ringwald

Axion-like particles (ALPs) are pseudo-scalar particles that are candidates for ultralight dark matter. ALPs interact with photons slightly and cause the rotational oscillation of linear polarization. DANCE searches for ALP dark matter by…

仪器与探测器 · 物理学 2021-05-19 Hiroki Fujimoto , Yuka Oshima , Masaki Ando , Tomohiro Fujita , Yuta Michimura , Koji Nagano , Ippei Obata

We use our recent electric dipole moment (EDM) measurement data to constrain the possibility that the HfF$^+$ EDM oscillates in time due to interactions with candidate dark matter axion-like particles (ALPs). We employ a Bayesian analysis…

We report on a broadband search for axion-like-particle (ALP) interactions using a radio-frequency-operated $^{87}\mathrm{Rb}$ atomic magnetometer. The instrument provides wide spectral coverage and sensitivity to an oscillating…

原子物理 · 物理学 2026-03-31 A. Rigoulet , S. Nanos , I. K. Kominis , D. Antypas