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We present a brief overview of recently proposed detection schemes for axion, axion-like pseudoscalar particle and topological defect dark matter. We focus mainly on the possibility of using atomic and molecular systems for dark matter…

High Energy Physics - Phenomenology · Physics 2014-11-26 Yevgeny V. Stadnik , Victor V. Flambaum

Axion dark matter (DM) is predicted to convert into radio waves in neutron star magnetospheres. We assess the detectability of this signal using a 5 m radio telescope to be installed at the Fan Mountain Observatory, operating in the UHF, L-…

We develop the theoretical model that describes dynamic non-equilibrium effects of external inertial and axion fields in a system of particles with spin. The possibility of using the spin density and the current density of non-relativistic…

High Energy Physics - Theory · Physics 2026-02-19 Mariya Iv. Trukhanova , Yuri N. Obukhov

Assuming for Weakly Interacting Massive Particles (WIMPs) a Maxwellian velocity distribution in the Galaxy we explore in a systematic way the relative sensitivity of an extensive set of existing and projected Dark Matter (DM) direct…

High Energy Physics - Phenomenology · Physics 2019-03-01 Sunghyun Kang , Stefano Scopel , Gaurav Tomar , Jong-Hyun Yoon

Axion-like particles (ALPs) arise from well-motivated extensions to the Standard Model and could account for the dark matter. We discuss the scaling of the sensitivity of a galactic ALP dark matter search with the number of sensors,…

High Energy Physics - Phenomenology · Physics 2025-04-18 Daniel Gavilan-Martin , Grzegorz Łukasiewicz , Derek F. Jackson Kimball , Szymon Pustelny , Dmitry Budker , Arne Wickenbrock

We report on a search for axion dark matter in the frequency range near 5.9 GHz, conducted using the haloscope technique. The experiment employed an 8-cell microwave resonator designed to extend the accessible frequency range by a…

Searches for dark matter scattering off nuclei are typically compared assuming that the dark matter's spin-independent couplings are identical for protons and neutrons. This assumption is neither innocuous nor well motivated. We consider…

High Energy Physics - Phenomenology · Physics 2011-10-18 Jonathan L. Feng , Jason Kumar , Danny Marfatia , David Sanford

The axion is a light pseudoscalar particle which suppresses CP-violating effects in strong interactions and also happens to be an excellent dark matter candidate. Axions constituting the dark matter halo of our galaxy may be detected by…

Traditional dark matter models, eg. WIMPs, assume dark matter is weakly coupled to the standard model so that elastic scattering between dark matter and baryons can be described perturbatively by Born approximation. Most direct detection…

High Energy Physics - Phenomenology · Physics 2021-12-03 Xingchen Xu , Glennys R. Farrar

We consider the proposal that dark matter (DM) is composed of a spin-3/2 particle that is a singlet of the standard model (SM). Its leading effective interactions with ordinary matter involve a pair of their fields and a pair of SM…

High Energy Physics - Phenomenology · Physics 2013-05-31 Ran Ding , Yi Liao , Ji-Yuan Liu , Kai Wang

The axion dark matter echo technique, proposed in Ref. [1], aims to search for axion dark matter by detecting the electromagnetic echo coming from stimulated decay of ambient axion dark matter interacting with a radio-microwave outgoing…

High Energy Physics - Phenomenology · Physics 2023-01-11 Ariel Arza , Abaz Kryemadhi , Konstantin Zioutas

We propose new ideas to directly search for light dark matter, such as the axion or the dark photon, by using magnetometry with nitrogen-vacancy centers in diamonds. If the dark matter couples to the electron spin, it affects the evolution…

High Energy Physics - Phenomenology · Physics 2025-03-17 So Chigusa , Masashi Hazumi , Ernst David Herbschleb , Norikazu Mizuochi , Kazunori Nakayama

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.…

The Cryogenic Dark Matter Search (CDMS) is an experiment to detect weakly interacting massive particles (WIMPs) based on their interactions with Ge and Si nuclei. We report the results of an analysis of data from the first two runs of CDMS…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

Conventional axion dark matter search experiments employ cylindrical microwave cavities immersed in a solenoidal magnetic field. Exploring higher frequency regions requires smaller size cavities as the TM010 resonant frequencies scale…

Instrumentation and Methods for Astrophysics · Physics 2017-11-29 Junu Jeong , SungWoo Youn , Saebyeok Ahn , Chanshin Kang , Yannis K. Semertzids

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…

Cosmological axions/axion-like particles can compose a significant part of dark matter; however, the uncertainty of their mass is large. Here, we propose to search the axions using a cylindrical capacitor, in which the static electric field…

High Energy Physics - Phenomenology · Physics 2024-06-21 Wenming Chen , Yu Gao , Qiaoli Yang

We propose to use the nuclear spin excitation in the ferromagnetic A1 phase of the superfluid $^3$He for the axion dark matter detection. This approach is striking in that it is sensitive to the axion-nucleon coupling, one of the most…

High Energy Physics - Phenomenology · Physics 2024-11-04 So Chigusa , Dan Kondo , Hitoshi Murayama , Risshin Okabe , Hiroyuki Sudo

We describe a resonant cavity search apparatus for axion dark matter constructed by the Quantum Sensors for the Hidden Sector (QSHS) collaboration. The apparatus is configured to search for QCD axion dark matter, though also has the…

We recently showed that macroscopic nuclear spin ensembles prepared in coherent spin states can dramatically enhance the interaction rates of weakly interacting cosmic relics-such as dark matter and the cosmic neutrino background-through…

High Energy Physics - Phenomenology · Physics 2026-05-01 Marios Galanis , Onur Hosten , Asimina Arvanitaki , Savas Dimopoulos