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相关论文: Opening the 1$\,$Hz axion window

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We study the formation of primordial black holes (PBHs) from density fluctuations due to supercooled phase transitions (PTs) triggered in an axion-like particle (ALP) model. We find that the mass of the PBHs is inversely correlated with the…

宇宙学与河外天体物理 · 物理学 2025-10-02 Angela Conaci , Luigi Delle Rose , P. S. Bhupal Dev , Anish Ghoshal

Axion-like particles (ALPs) with couplings to electromagnetism have long been postulated as extensions to the Standard Model. String theory predicts an "axiverse" of many light axions, some of which may make up the dark matter in the…

高能物理 - 唯象学 · 物理学 2019-07-17 Zachary Bogorad , Anson Hook , Yonatan Kahn , Yotam Soreq

We study the LHC phenomenology of an Axion Like Particle (ALP) that couples only derivatively with the top quark at tree level. We inspect the radiatively induced couplings with the SM fermions and (gauge) bosons and the associated…

高能物理 - 唯象学 · 物理学 2024-06-19 Simone Blasi , Fabio Maltoni , Alberto Mariotti , Ken Mimasu , Davide Pagani , Simone Tentori

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

The even light QCD axion called the $Z_{\mathcal N}$ axion can both solve the strong CP problem and account for the dark matter (DM). We point out that the single and double level crossings can naturally take place in the mass mixing…

高能物理 - 唯象学 · 物理学 2024-01-05 Hai-Jun Li , Ying-Quan Peng , Wei Chao , Yu-Feng Zhou

Adding an axion-like particle (ALP) to the Standard Model, with a field velocity in the early universe, simultaneously explains the observed baryon and dark matter densities. This requires one or more couplings between the ALP and photons,…

高能物理 - 唯象学 · 物理学 2021-02-24 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

Axion-like particles (ALPs) interacting with the Standard Model can be abundantly produced in proton beam fixed-target experiments. Looking for their displaced decays is therefore an effective search strategy for ALPs with a mass in the MeV…

高能物理 - 唯象学 · 物理学 2022-02-08 Nikita Blinov , Elizabeth Kowalczyk , Margaret Wynne

Axion-Like Particles (ALPs) are well-motivated candidates for dark matter and potential mediators to the dark sector. We present a search for ALPs coupled to photons, based on a reinterpretation of COMPASS data. Using the 2009 dataset…

高能物理 - 唯象学 · 物理学 2026-04-23 Mehran Dehpour

We study the mirror world with dark matter arising from the thermal freeze-out of the lightest, stable mirror particle -- the mirror electron. The dark matter abundance is achieved for mirror electrons of mass 225 GeV, fixing the mirror…

高能物理 - 唯象学 · 物理学 2023-02-10 David I. Dunsky , Lawrence J. Hall , Keisuke Harigaya

We show that very compact axion mini-clusters can form in models where axion-like-particle (ALP) dark matter is produced via the kinetic misalignment mechanism, which is well-motivated in pre-inflationary $U(1)$ symmetry breaking scenarios.…

高能物理 - 唯象学 · 物理学 2024-05-06 Cem Eröncel , Géraldine Servant

Axions and axion-like particles (ALPs) appear in many extensions of the Standard Model and are being investigated as promising dark matter (DM) candidates. One viable methodology for their detection involves the investigation of the…

高能天体物理现象 · 物理学 2024-04-18 Wen-Qing Guo , Zi-Qing Xia , Xiaoyuan Huang

Axion-like particles (ALPs) appear from spontaneous global symmetry breaking in many extensions of the Standard Model (SM). In this paper, we find bounds on ALP ($a$) model parameters at the LHC from the ALP production associated with a…

高能物理 - 唯象学 · 物理学 2019-07-24 Javad Ebadi , Sara Khatibi , Mojtaba Mohammadi Najafabadi

In this work, we present a lattice study of an axion - dark photon system in the early Universe and show that the stochastic gravitational wave (GW) background produced by this system may be probed by future GW experiments across a vast…

宇宙学与河外天体物理 · 物理学 2021-07-07 Wolfram Ratzinger , Pedro Schwaller , Ben A. Stefanek

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

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

Axion-like particles (ALPs) decaying into photons are known to affect a wide range of astrophysical and cosmological observables. In this study we focus on ALPs with masses in the keV-MeV range and lifetimes between $10^4$ and $10^{13}$…

The axion is a highly motivated elementary particle which could address two fundamental questions in physics - the strong CP problem and the dark matter mystery. Experimental searches for this hypothetical particle have started to reach…

高能物理 - 唯象学 · 物理学 2021-10-28 Yannis K. Semertzidis , SungWoo Youn

Ultra-light axion-like particles (ALPs) can be a viable solution to the dark matter problem. The scalar field associated with ALPs, coupled to the electromagnetic field, acts as an active birefringent medium, altering the polarisation…

Ultra-Light Axion-like Particle (ULAP) is motivated as one of the solutions to the small scale problems in astrophysics. When such a scalar particle oscillates with an $\mathcal{O}(1)$ amplitude in a potential shallower than quadratic, it…

宇宙学与河外天体物理 · 物理学 2022-10-26 Masahiro Kawasaki , Wakutaka Nakano , Hiromasa Nakatsuka , Eisuke Sonomoto

Axions solve the Strong CP Problem and are a cold dark matter candidate. The combined constraints from accelerator searches, stellar evolution limits and cosmology suggest that the axion mass is in the range $3 \cdot 10^{-3} > m_a >…

高能物理 - 唯象学 · 物理学 2007-05-23 Pierre Sikivie