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Related papers: A High Resolution Search for Dark-Matter Axions

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Axions are a well-motivated candidate for dark matter. The preeminent method to search for axion dark matter is known as the axion haloscope, which makes use of the conversion of axions to photons in a large magnetic field. Due to the weak…

We report an extensive high-sensitivity search for axion dark matter above 1\,GHz at the Center for Axion and Precision Physics Research (CAPP). The cavity resonant search, exploiting the coupling between axions and photons, explored the…

Axions are considered as a candidate of dark matter. The axions form coherent clouds which delay and amplify gravitational waves (GWs) at a resonant frequency. That is, the coherent axion clouds produce secondary GWs following a primary…

High Energy Physics - Phenomenology · Physics 2023-05-24 Takuya Tsutsui , Atsushi Nishizawa

The sensitivity of axion dark matter searches depends on the signal window that results from the velocity dispersion of axion dark matter. Since the ratio of signal windows is about 6500 between the standard halo and the big flow axion dark…

Cosmology and Nongalactic Astrophysics · Physics 2025-06-19 Andrew K. Yi , Byeong Rok Ko

Monochromatic high-frequency gravitational waves (HFGW) provide a distinctive probe of new physics scenarios, most notably axion clouds around rotating black holes formed via superradiance. We reanalyzed data from the CAPP-12T MC…

Context. Recent findings of line emission at 3.5 keV in both individual and stacked X-ray spectra of galaxy clusters have been speculated to have dark matter origin. Aims. If the origin is indeed dark matter, the emission line is expected…

Cosmology and Nongalactic Astrophysics · Physics 2016-05-18 Signe Riemer-Sorensen

The latest result from the ORGAN experiment, an axion haloscope is presented. This iteration of the experiment operated at millikelvin temperatures using a flux-driven Josephson parametric amplifier for reduced noise, along with various…

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…

We report a mm-wave search for axion dark matter from SGR 1745-2900, based on 4.8 h of ALMA observations. No candidate features are found between 133.99-135.78, 135.91-137.70, 145.99-147.78, and 147.99-149.78~GHz, corresponding to 0.55-0.62…

High Energy Physics - Phenomenology · Physics 2026-05-26 Javier De Miguel , Evanthia Hatziminaoglou , Frédéric Poidevin , Nanda Rea , Daniel L. Walker , Davide De Grandis , Jaime Prieto-Polo

Axions are one of the well-motivated candidates for dark matter, originally proposed to solve the strong CP problem in particle physics. Dark matter Axion search with riNg Cavity Experiment (DANCE) is a new experimental project to broadly…

The mass of axion dark matter is only weakly bounded by cosmological observations, necessitating a variety of detection techniques over several orders of magnitude of mass ranges. Axions haloscopes based on resonant cavities have become the…

Instrumentation and Detectors · Physics 2018-10-29 Ben T. McAllister , Maxim Goryachev , Jeremy Bourhill , Eugene N. Ivanov , Michael E. Tobar

About 30-50% of the baryons in the local Universe are unaccounted for and are likely in a hot phase, 10^5.5-10^8 K. A hot halo (10^6.3 K) is detected around the Milky Way through the O VII and O VIII resonance absorption and emission lines…

Astrophysics of Galaxies · Physics 2016-01-27 Joel N. Bregman , Guilherme Camargo Alves , Matthew J. Miller , Edmund Hodges-Kluck

CAPP-8TB is an axion dark matter search experiment dedicated to an axion mass search near 6.7 $\mu$eV. The experiment uses a microwave resonant cavity under a strong magnetic field of 8 T produced by a superconducting solenoid magnet in a…

Instrumentation and Detectors · Physics 2021-08-25 J. Choi , S. Ahn , B. R. Ko , S. Lee , Y. K. Semertzidis

We revisit birefringence effects associated with the evolution of the polarization of light as it propagates through axion dark matter or the background of a passing gravitational wave (GW). We demonstrate that this can be described by a…

High Energy Physics - Phenomenology · Physics 2025-01-16 Camilo García-Cely , Luca Marsili , Andreas Ringwald , Aaron D. Spector

Microwave cavities have been deployed to search for bosonic dark matter candidates with masses of a few $\mu$eV. However, the sensitivity of these cavity detectors is limited by their volume, and the traditionally-employed half-wavelength…

High Energy Physics - Experiment · Physics 2022-11-10 R. Cervantes , G. Carosi , C. Hanretty , S. Kimes , B. H. LaRoque , G. Leum , P. Mohapatra , N. S. Oblath , R. Ottens , Y. Park , G. Rybka , J. Sinnis , J. Yang

We report an axion dark matter search with a haloscope equipped with a microwave photon counter. The haloscope is a tunable high quality factor 3-dimensional microwave cavity placed in a magnetic field. The photon counter, operated…

This article reviews different microwave technologies used in dark matter axion detection experiments with resonant cavities. The general concepts of the experiment are presented and ways to optimize the design parameters of microwave…

Instrumentation and Detectors · Physics 2024-05-01 Jose R. Navarro-Madrid , Jose María García-Barceló , Alejandro Díaz-Morcillo

We present new results of a room temperature resonant AC haloscope, which searches for axions via photon upconversion. Traditional haloscopes require a strong applied DC magnetic background field surrounding the haloscope cavity resonator,…

High Energy Physics - Experiment · Physics 2023-06-08 Catriona A. Thomson , Maxim Goryachev , Ben T. McAllister , Eugene N. Ivanov , Paul Altin , Michael E. Tobar

The search for dark matter has been performed mainly for weakly interacting massive particles and massive compact halo objects, and the intermediate mass region has not been investigated experimentally. A method to search dark matter with…

Instrumentation and Detectors · Physics 2019-01-23 Akio Kawasaki

At low redshift, only about one-tenth of the known baryons lie in galaxies or the hot gas seen in galaxy clusters and groups. Models posit that these "missing baryons" are in gaseous form in overdense filaments that connect the much denser…

Astrophysics · Physics 2009-06-23 Joel N. Bregman
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