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Earth can act as a transducer to convert ultralight bosonic dark matter (axions and hidden photons) into an oscillating magnetic field with a characteristic pattern across its surface. Here we describe the first results of a dedicated…

Dark matter may consist of light, very weakly interacting bosons, produced non-thermally in the early Universe. Prominent examples of such very weakly interacting slim particles (WISPs) are axions and hidden photons. Direct detection…

High Energy Physics - Phenomenology · Physics 2013-12-16 Joerg Jaeckel , Javier Redondo

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

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

We propose a novel dark matter detection method utilizing the excitation of superconducting transmon qubits. Assuming the hidden photon dark matter of a mass of $O(10)\ \mu{\rm eV}$, the classical wave-matter oscillation induces an…

High Energy Physics - Phenomenology · Physics 2023-11-20 Shion Chen , Hajime Fukuda , Toshiaki Inada , Takeo Moroi , Tatsumi Nitta , Thanaporn Sichanugrist

We propose a new strategy to search for dark matter axions using tunable cryogenic plasmas. Unlike current experiments, which repair the mismatch between axion and photon masses by breaking translational invariance (cavity and dielectric…

High Energy Physics - Phenomenology · Physics 2019-10-02 Matthew Lawson , Alexander J. Millar , Matteo Pancaldi , Edoardo Vitagliano , Frank Wilczek

The search for dark matter and physics beyond the Standard Model has grown to encompass a highly interdisciplinary approach. In this review, we survey recent searches for light, weakly-coupled particles - axions and dark photons - over the…

High Energy Physics - Phenomenology · Physics 2024-12-13 Asher Berlin , Yonatan Kahn

We introduce the Broadband Reflector Experiment for Axion Detection (BREAD) conceptual design and science program. This haloscope plans to search for bosonic dark matter across the [10$^{-3}$, 1] eV ([0.24, 240] THz) mass range. BREAD…

Dark matter experiments primarily search for the scattering of WIMPs on target nuclei of well shielded underground detectors. The results from liquid scintillator experiments furthermore provide precise probes of very light and very weakly…

High Energy Physics - Phenomenology · Physics 2015-10-19 Haipeng An , Kaixuan Ni , Maxim Pospelov , Josef Pradler , Adam Ritz

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…

Dark photons (DPs) produced in the early Universe are well-motivated dark matter (DM) candidates. We show that the recently proposed tunable plasma haloscopes are particularly advantageous for DP searches. While in-medium effects suppress…

High Energy Physics - Phenomenology · Physics 2020-08-12 Graciela B. Gelmini , Alexander J. Millar , Volodymyr Takhistov , Edoardo Vitagliano

Among laboratory probes of dark matter, fixed-target neutrino experiments are particularly well-suited to search for light weakly-coupled dark sectors. In this paper, we show that the DAEdALUS source setup---an 800 MeV proton beam impinging…

High Energy Physics - Phenomenology · Physics 2015-03-13 Yonatan Kahn , Gordan Krnjaic , Jesse Thaler , Matthew Toups

Dark matter (DM) with masses of order an electronvolt or below can have a non-zero coupling to electromagnetism while being compatible with cosmological observations. In these models, the ambient DM behaves as a new classical source in…

High Energy Physics - Phenomenology · Physics 2026-02-23 Nikita Blinov , Christina Gao , Roni Harnik , Ryan Janish , Neil Sinclair

Dark matter particles with a mass around 1 eV can decay into near-infrared photons. Utilising available public blank sky observations from the NIRSpec IFU on the James Webb Space Telescope (JWST), we search for a narrow emission line due to…

High Energy Physics - Phenomenology · Physics 2023-10-25 Ryan Janish , Elena Pinetti

The dark photon is a new hypothetical gauge boson arising in extensions of the Standard Model, and constitutes a compelling dark matter candidate. As dark photon dark matter (DPDM), it can interact with electromagnetic fields via kinetic…

High Energy Astrophysical Phenomena · Physics 2026-02-26 Júlia G. Mamprim , Aion Viana , Vitor de Souza

Establishing the axion as the dark matter (DM) particle after a haloscope discovery typically requires follow-up experiments to break the degeneracy between the axion's coupling to photons and its local DM abundance. Given that a discovery…

High Energy Physics - Phenomenology · Physics 2025-01-09 Sebastian Hoof , Joerg Jaeckel , Giuseppe Lucente

Axion Dark Matter eXperiment (ADMX) ultra low noise haloscope technology has enabled the successful completion of two science runs (1A and 1B) that looked for dark matter axions in the $2.66$ to $3.1$ $\mu$eV mass range with…

Collective excitations in condensed matter systems, such as phonons and magnons, have recently been proposed as novel detection channels for light dark matter. We show that excitation of i) optical phonon polaritons in polar materials in an…

High Energy Physics - Phenomenology · Physics 2020-11-11 Andrea Mitridate , Tanner Trickle , Zhengkang Zhang , Kathryn M. Zurek

We propose new concepts for experiments in which intense high energy photon or muon beams are employed parasitically to detect scattering by cosmic heavy weakly interacting dark matter (DM) particles. We show that the scattering…

High Energy Physics - Phenomenology · Physics 2026-03-04 A. Acar , M. Bashkanov , D. P. Watts
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