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相关论文: Composite heavy axion-like dark matter

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We establish strong gravitational lens systems as robust probes of axion-like particles (ALPs) -- a candidate for dark matter. A tiny interaction of photons with ALPs induces birefringence. Multiple images of gravitationally lensed…

宇宙学与河外天体物理 · 物理学 2021-05-19 Aritra Basu , Jishnu Goswami , Dominik J. Schwarz , Yuko Urakawa

We review models of new physics in which dark matter arises as a composite bound state from a confining strongly-coupled non-Abelian gauge theory. We discuss several qualitatively distinct classes of composite candidates, including dark…

高能物理 - 唯象学 · 物理学 2016-08-24 Graham D. Kribs , Ethan T. Neil

We report on the first results of the Noble and Alkali Spin Detectors for Ultralight Coherent darK matter (NASDUCK) collaboration. We search for the interactions of Axion-Like Particles (ALPs) with atomic spins using an earth-based…

高能物理 - 唯象学 · 物理学 2022-02-08 Itay M. Bloch , Gil Ronen , Roy Shaham , Ori Katz , Tomer Volansky , Or Katz

An axion-like particle (ALP) with mass $m_\phi \sim 10^{-15}$eV oscillates with frequency $\sim$1 Hz. This mass scale lies in an open window of astrophysical constraints, and appears naturally as a consequence of grand unification (GUT) in…

高能物理 - 唯象学 · 物理学 2021-01-06 David J. E. Marsh , Wen Yin

Galactic dark matter may consist of axionlike particles (ALPs) that can be described as an "ultralight bosonic field" oscillating at the ALP Compton frequency. The ALP field can be searched for using nuclear magnetic resonance (NMR), where…

Heavy axion-like particles (ALPs), with masses up to a few 100 keV and coupled with photons can be efficiently produced in stellar plasmas, contributing to a significant energy-loss. This argument has been applied to helium burning stars in…

高能物理 - 唯象学 · 物理学 2022-06-30 Giuseppe Lucente , Oscar Straniero , Pierluca Carenza , Maurizio Giannotti , Alessandro Mirizzi

Axion-like particles (ALPs) are a compelling candidate for dark matter (DM), whose production is associated with the formation of a string-wall network. If walls bounded by strings persist, which requires the potential to have multiple…

高能物理 - 唯象学 · 物理学 2021-09-29 Graciela B. Gelmini , Anna Simpson , Edoardo Vitagliano

Axion-like particles (ALPs) are a well-motivated dark matter candidate that solve some of the problems in the clustering of large scale structure in cosmology. ALPs are often described by a simplified quadratic potential to specify the…

宇宙学与河外天体物理 · 物理学 2024-06-13 Harrison Winch , Renee Hlozek , David J. E. Marsh , Daniel Grin , Keir Rogers

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 highly viable candidates for dark matter (DM) in the universe. If…

高能天体物理现象 · 物理学 2019-11-25 Ahmed Ayad , Geoff Beck

Assuming that dark matter is an ultralight pseudoscalar particle which couples to electromagnetism like an axion (an ALP), we demonstrate that the coupling of the cosmological magnetic field produced by the ALP field oscillations to the…

高能物理 - 唯象学 · 物理学 2026-02-26 Ashu Kushwaha , Robert Brandenberger

The QCD axion was originally predicted as a dynamical solution to the strong CP problem. Axion like particles (ALPs) are also a generic prediction of many high energy physics models including string theory. Theoretical models for axions are…

高能物理 - 唯象学 · 物理学 2017-12-11 David J. E. Marsh

The dark axion portal is a dimension-5 coupling between an axion-like particle (ALP), a photon, and a dark photon, which is one of the targets of the intensity frontier searches looking for $\sim\,$sub-GeV long-lived particles (LLPs). In…

高能物理 - 唯象学 · 物理学 2023-05-18 Krzysztof Jodłowski

We study the effective Lagrangian for the Axion-Like Particle (ALP) arising in a class of composite Higgs models. We discuss the peculiarities of the coupling to the quark sector specific of these models, including flavor violating terms.…

高能物理 - 唯象学 · 物理学 2025-07-08 Gabriele Ferretti

Dark matter (DM) can be composed of a collection of axions, or axion-like particles (ALPs), whose existence is due to the spontaneous breaking of the Peccei-Quinn $U(1)$ symmetry which is the most compelling solution of the strong…

高能物理 - 唯象学 · 物理学 2023-06-16 Bryan Cordero-Patino , Álvaro Duenas-Vidal , Jorge Segovia

Axion Like Particles (ALPs) belong to a well motivated class of particles which are part of a more complete UV theory. In this work, we initiate and present the inclusion of such ALPs or the conventional axions in the Heavy Hadron Chiral…

高能物理 - 唯象学 · 物理学 2023-08-02 Namit Mahajan

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…

Dark matter may consist of axion-like particles (ALPs). When polarized electromagnetic radiation passes through the dark-matter media, interaction with background ALPs affects the polarization of photons. The condensate of axionic dark…

高能物理 - 唯象学 · 物理学 2025-05-02 D. Davydov , Alexander Libanov

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

Axion-like particles (ALPs) can account for the observed dark matter (DM) of the Universe and if their masses are at the eV scale, they can decay into infrared, optical and ultraviolet photons with a decay lifetime larger than the age of…

高能物理 - 唯象学 · 物理学 2025-06-03 Arpan Kar , Sourov Roy , Pratick Sarkar

Hypothetical axion-like particles (ALPs) are of interest because of their potential to act as dark matter or to reveal information about yet undiscovered fundamental constituents of matter. Such particles can be created when photons…

高能天体物理现象 · 物理学 2025-08-19 Denys Malyshev , Lidiia Zadorozhna , Yuriy Bidasyuk , Andrea Santangelo , Oleg Ruchayskiy