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An absorption dip in the spectrum of the cosmic microwave background observed by the EDGES experiment suggests an unexplained reduction of the hydrogen spin temperature at cosmic redshift z ~ 17. The mass of dark-matter axions could…

高能物理 - 唯象学 · 物理学 2019-01-23 Adrien Auriol , Sacha Davidson , Georg Raffelt

Dark matter axions may cause transitions between atomic states that differ in energy by an amount equal to the axion mass. Such energy differences are conveniently tuned using the Zeeman effect. It is proposed to search for dark matter…

高能物理 - 唯象学 · 物理学 2020-06-02 P. Sikivie

Hidden axions may be coupled to the standard model particles through a kinetic or mass mixing with QCD axion. We study a scenario in which a hidden axion constitutes a part of or the whole of dark matter and decays into photons through the…

高能物理 - 唯象学 · 物理学 2015-06-22 Tetsutaro Higaki , Naoya Kitajima , Fuminobu Takahashi

Current techniques cannot detect axion dark matter over much of its parameter space, particularly in the theoretically well-motivated region where the axion decay constant f_a lies near the GUT and Planck scales. We suggest a novel…

高能物理 - 唯象学 · 物理学 2011-10-03 Peter W. Graham , Surjeet Rajendran

The QCD axion is a promising candidate of the dark matter. In this paper, we discuss elastic scattering processes between nucleons and the QCD axion dark matter. We point out that the cross section can be enhanced by more than…

高能物理 - 唯象学 · 物理学 2022-06-01 Hajime Fukuda , Satoshi Shirai

A light hidden photon or axion-like particle is a good dark matter candidate and they are often associated with the spontaneous breaking of dark global or gauged U(1) symmetry. We consider the dark Higgs dynamics around the phase transition…

高能物理 - 唯象学 · 物理学 2021-10-27 Kazunori Nakayama , Wen Yin

A QCD axion with a decay constant below $ 10 ^{ 11} ~{\rm GeV} $ is a strongly-motivated extension to the Standard Model, though its relic abundance from the misalignment mechanism or decay of cosmic defects is insufficient to explain the…

高能物理 - 唯象学 · 物理学 2023-06-07 Jeff Dror , Stefania Gori , Pankaj Munbodh

The QCD axion is a good dark matter candidate. The observed dark matter abundance can arise from misalignment or defect mechanisms, which generically require an axion decay constant $f_a \sim \mathcal{O}(10^{11})$ GeV (or higher). We…

高能物理 - 唯象学 · 物理学 2018-07-27 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

We investigate the level-crossing phenomenon in two-axion systems, where the mass eigenvalues intersect as the mass of one axion increases with the cooling of the universe. This phenomenon can significantly alter the abundance of axions in…

高能物理 - 唯象学 · 物理学 2024-12-16 Kai Murai , Yuma Narita , Fuminobu Takahashi , Wen Yin

We propose an approach to search for axion dark matter with a specially designed superconducting radio frequency cavity, targeting axions with masses $m_a \lesssim 10^{-6} \text{ eV}$. Our approach exploits axion-induced transitions between…

The dark matter puzzle is one of the most important open problems in modern physics. The ultra-light axion is a well-motivated dark matter candidate, conceived to resolve the strong-CP problem of quantum chromodynamics. Numerous precision…

高能物理 - 唯象学 · 物理学 2023-07-24 Alexander O. Sushkov

Axion-like fields are naturally generated by a mechanism of anomaly cancellation of one or more anomalous gauge abelian symmetries at the Planck scale, emerging as duals of a two-form from the massless bosonic sector of string theory. This…

高能物理 - 唯象学 · 物理学 2018-07-04 Claudio Coriano , Paul H. Frampton

The QCD axion or axion-like particles are candidates of dark matter of the universe. On the other hand, axion-like excitations exist in certain condensed matter systems, which implies that there can be interactions of dark matter particles…

高能物理 - 唯象学 · 物理学 2021-09-01 So Chigusa , Takeo Moroi , Kazunori Nakayama

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

Dark matter in the form of axions is expected to form miniclusters, and their dense regions can harbor compact axion stars. Such axion stars could be discovered by microlensing events. In particular, some candidate events reported by Subaru…

高能物理 - 唯象学 · 物理学 2023-04-10 Sunao Sugiyama , Masahiro Takada , Alexander Kusenko

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

Existence of dark matter indicates the presence of unknown fundamental laws of nature. Ultralight axion-like particles are well-motivated dark matter candidates, emerging naturally from theories of physics at ultrahigh energies. We report…

高能物理 - 实验 · 物理学 2021-01-11 Alexander V. Gramolin , Deniz Aybas , Dorian Johnson , Janos Adam , Alexander O. Sushkov

Recently, two of the present authors showed that even when the axion momentum is much smaller than its mass, the axion can still behave like radiation if its energy density greatly exceeds the maximum potential energy set by the cosine-type…

高能物理 - 唯象学 · 物理学 2025-09-17 Max Miyazaki , Yuma Narita , Deheng Song , Nemin Yaginuma , Wen Yin

We report on a search for ultra-low-mass axion-like dark matter by analysing the ratio of the spin-precession frequencies of stored ultracold neutrons and $^{199}$Hg atoms for an axion-induced oscillating electric dipole moment of the…

We study the atomic physics and the astrophysical implications of a model in which the dark matter is the analog of hydrogen in a secluded sector. The self interactions between dark matter particles include both elastic scatterings as well…

高能物理 - 唯象学 · 物理学 2017-01-11 Kimberly K. Boddy , Manoj Kaplinghat , Anna Kwa , Annika H. G. Peter
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