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The interaction between axion-like particles (ALPs) and photons induces ALP-photon oscillations in astrophysical magnetic fields, leading to spectral distortions in the $\gamma$-ray spectrum of blazars. The primary uncertainty of this…

高能天体物理现象 · 物理学 2024-07-30 Lin-Qing Gao , Xiao-Jun Bi , Jun Li , Peng-Fei Yin

We demonstrate that enhanced early galaxy formation can generically arise in axion-like particle (ALP) dark matter (DM) models with a delayed onset of axion field oscillation. In these models, the formation of localized massive objects…

高能物理 - 唯象学 · 物理学 2024-10-16 Simeon Bird , Chia-Feng Chang , Yanou Cui , Daneng Yang

We consider a cosmological scenario in which the very early Universe experienced a transient epoch of matter domination due to the formation of a large population of primordial black holes (PBHs) with masses $M \lesssim 10^{9}\,\textrm{g}$,…

高能物理 - 唯象学 · 物理学 2021-09-03 Francesco Schiavone , Daniele Montanino , Alessandro Mirizzi , Francesco Capozzi

Axions and axion-like particles (ALPs) are some of the most popular candidates for dark matter, with several viable production scenarios that make different predictions. In the scenario in which the axion is born after inflation, its field…

高能物理 - 唯象学 · 物理学 2022-03-31 Ciaran A. J. O'Hare , Giovanni Pierobon , Javier Redondo , Yvonne Y. Y. Wong

We show that dark matter can be accounted for by an axion that solves the strong CP problem, but is much lighter than usual due to a $Z_\mathcal{N}$ symmetry. The whole mass range from the canonical QCD axion down to the ultra-light regime…

高能物理 - 唯象学 · 物理学 2023-02-16 Luca Di Luzio , Belen Gavela , Pablo Quilez , Andreas Ringwald

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

Many works have concentrated on the observable signatures of the dark matter being an ultralight axion-like particle (ALP). We concentrate on a particularly dramatic signature in the late-time cosmological matter power spectrum that occurs…

宇宙学与河外天体物理 · 物理学 2020-06-24 Vid Iršič , Huangyu Xiao , Matthew McQuinn

Recently it has been pointed out that a cosmic background of relativistic axion-like particles (ALPs) would be produced by the primordial decays of heavy fields in the post-inflation epoch, contributing to the extra-radiation content in the…

宇宙学与河外天体物理 · 物理学 2016-05-25 Carmelo Evoli , Matteo Leo , Alessandro Mirizzi , Daniele Montanino

The Axion Like Particle (ALP) is a hypothetical pseudo-scalar particle beyond the Standard Model, with a compelling possible connection to dark matter and early universe physics. ALPs can be converted into photons via interactions with…

高能天体物理现象 · 物理学 2020-03-04 Ryo Yamamoto , Noriko Y. Yamasaki , Kazuhisa Mitsuda , Masahiro Takada

Although axion-like particles (ALPs) are popular dark matter candidates, their mass generation mechanisms as well as cosmic thermal evolutions are still unclear. In this letter, we propose a new mass generation mechanism of ALP during the…

高能物理 - 唯象学 · 物理学 2022-10-25 Wei Chao , Mingjie Jin , Hai-Jun Li , Ying-Quan Peng

We propose a mechanism generating primordial magnetic fields after the $e^+e^-$ annihilations. Our mechanism involves an ultra-light axion-like particle (ALP) which constitutes the dark matter, and a dark $U(1)_X$ gauge boson introduced to…

高能物理 - 唯象学 · 物理学 2018-07-25 Kiwoon Choi , Hyungjin Kim , Toyokazu Sekiguchi

We present constraints on the nature of axions and axionlike particles (ALPs) by analyzing gamma--ray data from neutron stars using the Fermi Large Area Telescope. In addition to axions solving the strong CP problem of particle physics,…

高能天体物理现象 · 物理学 2016-03-02 Bijan Berenji , Jennifer Gaskins , Manuel Meyer

We investigate the role of an axion-like particle (ALP) as a portal between the dark and visible sectors. Unlike conventional studies, which typically assume fermionic dark matter (DM), we explore the phenomenological implications of scalar…

高能物理 - 唯象学 · 物理学 2025-07-08 Francesco D'Eramo , Tommaso Sassi

Cosmic birefringence, characterized by the observed rotation of the polarization plane of the cosmic microwave background (CMB) radiation, serves as a critical probe for testing theories beyond the standard cosmological scenario. As a major…

宇宙学与河外天体物理 · 物理学 2025-12-29 Jialiang Shao , Ippei Obata , Dongdong Zhang

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

Cosmological data provides us two key constraints on dark matter (DM): it must have a particular abundance, and it must have an adiabatic spectrum of density perturbations in the early universe. Many different cosmological scenarios have…

高能物理 - 唯象学 · 物理学 2025-10-28 Itamar J. Allali , Priyesh Chakraborty , JiJi Fan , Matthew Reece

Understanding axion production in the early Universe remains a pivotal challenge, given the axion as a compelling cold dark matter candidate. Conventional misalignment scenarios often overlook the possibility that a large initial axion…

高能物理 - 唯象学 · 物理学 2026-04-03 Wei Chao , Chang-Jie Dai

If axion-like particles (ALPs) constitute a major part of dark matter (DM), due to the bosonic nature and a relative small mass, they could behave differently from the point like dark matter particles on the formation of the cosmic…

高能物理 - 唯象学 · 物理学 2017-04-11 Qiaoli Yang , Haoran Di

Axion-like particles (ALPs) arise from well-motivated extensions to the Standard Model and could account for dark matter. ALP dark matter would manifest as a field oscillating at an (as of yet) unknown frequency. The frequency depends…

Axion-like particles (ALPs) are interesting dark matter candidates both from the theoretical as well as from the experimental perspective. Usually they are motivated as pseudo-Nambu-Goldstone bosons. In this case one of their most important…

高能物理 - 唯象学 · 物理学 2018-08-01 Gonzalo Alonso-Álvarez , Joerg Jaeckel