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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…

High Energy Physics - Phenomenology · Physics 2022-06-01 Hajime Fukuda , Satoshi Shirai

We search for dark matter in the form of axionlike particles (ALPs) in the mass range $5.576741 \,\mathrm{neV/c^2}$ - $5.577733\,\mathrm{neV/c^2}$ by probing their possible coupling to fermion spins through the ALP field gradient. This is…

It has been hypothesized that dark matter is comprised of ultra-light bosons whose collective phenomena can be described as a scalar field undergoing coherent oscillations. Examples include axion and fuzzy dark matter models. In this…

High Energy Physics - Phenomenology · Physics 2023-05-08 Jeremy Sakstein , Ippocratis D. Saltas

The investigation on the production of particles in slowly varying but extremely intense magnetic field in extended to the case of axions. The motivation is, as for some previously considered cases, the possibility that such kind of…

High Energy Physics - Phenomenology · Physics 2008-11-26 Giorgio Calucci

The search for axions has gained ground in recent years, with laboratory searches for cold dark matter (CDM) axions, relativistic solar axions and ultra-light axions the subject of extensive literature. In particular, the interest in axions…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-07 Katharine Kelley , P. J. Quinn

A number of proposals have been put forward for detecting axion dark matter (DM) with grand unification scale decay constants that rely on the conversion of coherent DM axions to oscillating magnetic fields in the presence of static,…

High Energy Physics - Phenomenology · Physics 2023-08-16 Joshua N. Benabou , Joshua W. Foster , Yonatan Kahn , Benjamin R. Safdi , Chiara P. Salemi

A ferromagnetic axion haloscope searches for Dark Matter in the form of axions by exploiting their interaction with electronic spins. It is composed of an axion-to-electromagnetic field transducer coupled to a sensitive rf detector. The…

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…

High Energy Physics - Phenomenology · Physics 2023-04-10 Sunao Sugiyama , Masahiro Takada , Alexander Kusenko

Light scalar and pseudoscalar particles are compelling dark matter candidates, with a vast running experimental program to discover them. Previous studies have shown that these light fields can generate sizable isocurvature perturbations in…

High Energy Physics - Phenomenology · Physics 2023-06-02 Andrea Caputo , Michael Geller , Giuseppe Rossi

It is known that a coherently oscillating axion field is a candidate of the dark matter. In the presence of the oscillating axion, the photon can be resonantly produced through the parametric amplification. In the universe, there also exist…

High Energy Physics - Phenomenology · Physics 2020-02-12 Emi Masaki , Arata Aoki , Jiro Soda

An argument is presented that the dark matter is axions, at least in part. It has three steps. First, axions behave differently from the other forms of cold dark matter because they form a rethermalizing Bose-Einstein condensate (BEC).…

Cosmology and Nongalactic Astrophysics · Physics 2012-10-02 P. Sikivie

Magnetic field dependent transient solar observations are suggestive for axion-photon oscillations with light axion(-like) particle involvement. Novel dark-moon measurements with the SMART X-ray detectors can be conclusive for radiatively…

We introduce and study a model designed to simultaneously shed light on the mysteries connected with Baryogenesis, Dark Matter and Dark Energy. The model describes a self-interacting complex axion field whose imaginary part, a pseudo-scalar…

High Energy Physics - Theory · Physics 2021-04-21 Robert Brandenberger , Jürg Fröhlich

Theoretical arguments predict that the distribution of cold dark matter in spiral galaxies has peaks in velocity space associated with non-thermalized flows of dark matter particles. We searched for the corresponding peaks in the spectrum…

We present an overview of recent developments in the detection of light bosonic dark matter, including axion, pseudoscalar axion-like and scalar dark matter, which form either a coherently oscillating classical field or topological defects…

Atomic Physics · Physics 2015-09-04 Y. V. Stadnik , V. V. Flambaum

We propose a mechanism for the generation of a magnetic field in the early universe during the QCD crossover assuming that dark matter is made of axions. Thermoelectric fields arise at pressure gradients in the primordial plasma due to the…

Cosmology and Nongalactic Astrophysics · Physics 2018-07-18 Francesco Miniati , Gianluca Gregori , Brian Reville , Subir Sarkar

The detection of dark matter is a challenging problem in modern physics. The ultralight scalar and axion dark matter could induce the oscillation of the nuclear charge radii and then oscillate the atomic transition frequency by interacting…

High Energy Physics - Phenomenology · Physics 2024-01-31 Wei Zhao , Hui Liu , Xitong Mei

Axions are possible candidates of dark matter in the present Universe. They have been argued to form axionic boson stars with small masses $10^{-14}M_{\odot}\sim 10^{-11}M_{\odot}$. Since they possess oscillating electric fields in a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Aiichi Iwazaki

The nature of dark matter, the invisible substance making up over $80\%$ of the matter in the Universe, is one of the most fundamental mysteries of modern physics. Ultralight bosons such as axions, axion-like particles or dark photons could…

Levitated sensors have emerged as a new frontier to detect ultra-light dark matter such as axion-like particles and dark photons. In this work we study how a magnetically levitated superconductor responds to a spin-2 dark matter field, the…

High Energy Physics - Phenomenology · Physics 2026-04-01 Valentina Danieli , Paola C. M. Delgado , Federico R. Urban