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A new search strategy for the detection of the elusive dark matter (DM) axion is proposed. The idea is based on streaming DM axions, whose flux might get temporally enormously enhanced due to gravitational lensing. This can happen if the…

Dark matter is a major constituent of our universe and the axion is a prime candidate. In this article, it is shown that by exploiting the axion induced magnetization in a magnetic rod and the Faraday effect, axions in the mass range $500$…

Cosmology and Nongalactic Astrophysics · Physics 2022-12-06 A. T. M. Anishur Rahman

The frequency band 1-15 GHz provides exciting prospects for resonant axion haloscopes as indicated by cosmological and astrophysical arguments. Among the challenges currently addressed to reach the required sensitivity, the development of…

Experiments aimed at detecting ultralight dark matter typically rely on resonant effects, which are sensitive to the dark matter mass that matches the resonance frequency. In this study, we investigate the nucleon couplings of ultralight…

High Energy Physics - Phenomenology · Physics 2024-07-12 Zitong Xu , Xiaolin Ma , Kai Wei , Yuxuan He , Xing Heng , Xiaofei Huang , Tengyu Ai , Jian Liao , Wei Ji , Jia Liu , Xiao-Ping Wang , Dmitry Budker

Dark matter Axion search with riNg Cavity Experiment (DANCE) was proposed to search for axion dark matter [Phys. Rev. Lett. 121, 161301 (2018)]. We aim to detect the rotation and oscillation of optical linear polarization caused by…

The natural environment of the Earth can act as a sensitive detector for dark matter in ultralight axions. When axions with masses between $1\times10^{-15}\,{\rm eV}$ and $1\times10^{-13}\,{\rm eV}$ pass through the Earth, they interact…

High Energy Physics - Phenomenology · Physics 2025-04-23 Atsushi Nishizawa , Atsushi Taruya , Yoshiaki Himemoto

Axions are well motivated particles proposed in an extension of the SM as a solution to the strong CP problem. Also, there is the category of Axion-Like Particles (ALPs) which appear in extensions of the SM and share the same phenomenology…

Solar and Stellar Astrophysics · Physics 2015-06-09 Juan Antonio García

The axion particle, a consequence of an elegant hypothesis that resolves the strong-CP problem of quantum chromodynamics, is a plausible origin for cosmological dark matter. In searches for axionic dark matter that detect the conversion of…

High Energy Physics - Phenomenology · Physics 2016-07-20 Huaixiu Zheng , Matti Silveri , R. T. Brierley , S. M. Girvin , K. W. Lehnert

We describe a novel search strategy for axions (or hadronically coupled axion-like particles) in the mass range of $m_a \lesssim 350\,{\rm MeV}$. The search relies on kaon decay at rest, which produces a mono-energetic signal in a large…

High Energy Physics - Phenomenology · Physics 2024-09-04 Yohei Ema , Zhen Liu , Ryan Plestid

The axion is a hypothetical particle proposed to solve the strong $CP$ problem, and also a candidate for dark matter. This non-relativistic particle in the galactic halo can be converted into a photon under a strong magnetic field and…

High Energy Physics - Experiment · Physics 2019-10-15 Soohyung Lee , Saebyeok Ahn , Jihoon Choi , Byeong Rok Ko , Yannis K. Semertzidis

We study the feasibility of a new generation axion helioscope, the most ambitious and promising detector of solar axions to date. We show that large improvements in magnetic field volume, x-ray focusing optics and detector backgrounds are…

We report a methodology to determine the quality factor ($Q$) in implementations of the so-called dielectric haloscope, a new concept of wavy dark matter detector equipped with a multilayered resonator. An anechoic chamber enables the…

The QCD axion is one of the most compelling candidates to explain the dark matter abundance of the universe. With its extremely small mass ($\ll 1\,\mathrm{eV}/c^2$), axion dark matter interacts as a classical field rather than a particle.…

We investigate the use of next generation radio telescopes such as the Square Kilometre Array (SKA) to detect axion two-photon coupling in the astrophysical environment. The uncertainty surrounding astrophysical magnetic fields presents new…

Cosmology and Nongalactic Astrophysics · Physics 2017-10-31 Katharine Kelley , P. J. Quinn

We describe the design of the dark matter experiment Haloscope At Yale Sensitive To Axion Cold Dark Matter (HAYSTAC), and report the results of a haloscope search for dark matter axions. We exclude axion models with axion-photon couplings…

Instrumentation and Detectors · Physics 2019-01-15 Alex G. Droster , Karl van Bibber

We develop a formalism to describe extensions of existing axion haloscope designs to those that possess directional sensitivity to incoming dark matter axion velocities. The effects are measurable if experiments are designed to have…

Cosmology and Nongalactic Astrophysics · Physics 2018-12-04 Stefan Knirck , Alexander J. Millar , Ciaran A. J. O'Hare , Javier Redondo , Frank D. Steffen

Axion dark matter searches use a microwave cavity for the resonant conversion of axions into photons to enhance experimental sensitivity, with the cavity generally configured as a two-port system for both signal pickup and cavity…

High Energy Physics - Phenomenology · Physics 2026-04-21 Byeong Rok Ko

We report the results of a search for dark photon dark matter using a cavity that employs a transmon qubit as a frequency tuner. The tuning mechanism utilizes the energy level shift arising from the mode mixing between the qubit and the…

Signal estimates for direct axion dark matter searches have used the isothermal sphere halo model for the last several decades. While insightful, the isothermal model does not capture effects from a halo's infall history nor the influence…

Astrophysics of Galaxies · Physics 2017-08-30 Erik W. Lentz , Thomas R. Quinn , Leslie J Rosenberg , Michael J. Tremmel

When axion cold dark matter interacts with a static magnetic field, it can be converted to photons with energy near the axion's mass. Classical analysis shows that incorporating a resonant cavity significantly enhances this conversion rate,…

High Energy Physics - Phenomenology · Physics 2025-05-20 Ruifeng Zheng , Puxian Wei , Qiaoli Yang
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