English
Related papers

Related papers: Echo-free quality factor of a multilayer axion hal…

200 papers

The axion offers a well-motivated solution to two fundamental questions in modern physics: the strong CP problem and the dark matter mystery. Cavity haloscopes, exploiting resonant enhancement of photon signals, provide the most sensitive…

Instrumentation and Detectors · Physics 2024-06-04 SungWoo Youn , Junu Jeong , Yannis K. Semertzidis

An analysis is provided of the degradation that arises in the quality factor of a whispering gallery mode when a circular or spherical dielectric cavity is deformed. The large quality factors of such resonators are important to their use in…

Optics · Physics 2015-06-04 Michael M. White , Stephen C. Creagh

The dark (or hidden) photon is a massive U(1) gauge boson theorized as a dark force mediator and as a dark matter candidate. Dark photons can be detected with axion cavity haloscopes by probing for a power excess caused by the dark photon's…

High Energy Physics - Phenomenology · Physics 2021-12-01 Sumita Ghosh , Liz Ruddy , Michael J. Jewell , Alexander F. Leder , Reina H. Maruyama

We demonstrate the active tuning of all-dielectric metasurfaces exhibiting high-quality factor (high-Q) resonances. The active control is provided by embedding the asymmetric silicon meta-atoms with liquid crystals, which allows the…

Quantum fluctuations constitute the primary noise barrier limiting cavity-based axion dark matter searches. In an experiment designed to mimic a real axion search, we employ a quantum-enhanced sensing technique to detect a synthetic…

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

Dark matter makes up 85% of the matter in the universe and 27% of its energy density, but we do not know what comprises dark matter. It is possible that dark matter may be composed of either axions or dark photons, both of which can be…

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 introduce the FLASH haloscope experiment and present its electronic read-out system, currently under development. FLASH searches for Dark Matter (DM) particles and High-Frequency Gravitational Waves (HFGWs) using two cryogenic resonant…

Instrumentation and Detectors · Physics 2026-05-07 Luigi Calligaris , Claudio Puglia , Gianluca Lamanna

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…

An integrated photonic platform is proposed for strong interactions between atomic beams and annealing-free high-quality-factor (Q) microresonators. We fabricated a thin-film, air-clad SiN microresonator with a loaded Q of $1.55\times10^6$…

Optics · Physics 2022-04-05 Ali Eshaghian Dorche , Bochao Wei , Chandra Raman , Ali Adibi

We show analytically that the quality ($Q$) factor of magnetic and electric Mie modes in a lossless dielectric spherical resonator with high refractive index ($n \gg 1$) scales as $n^{2j+1}$ and $n^{2j+3}$ respectively, where $j$ denotes…

Optics · Physics 2025-02-14 Xavier Zambrana-Puyalto , Søren Raza

Axions or axion-like particles (ALPs) are one of the promising dark matter (DM) candidates. A prevalent method to detect axion-like DM is to seek periodic oscillation in the polarization angles (PAs) of linearly polarized light emitted from…

High Energy Astrophysical Phenomena · Physics 2025-04-03 Bao Wang , Xuan Yang , Jun-Jie Wei , Song-Bo Zhang , Xue-Feng Wu

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

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…

We argue that dielectric haloscopes like MADMAX, originally designed for detecting axion dark matter, are also very promising gravitational wave detectors. Operated in resonant mode at frequencies around $\mathcal{O}(10\,\text{GHz})$, these…

High Energy Physics - Phenomenology · Physics 2024-09-11 Valerie Domcke , Sebastian A. R. Ellis , Joachim Kopp

The dark photon is a well motivated candidate for the dark matter which comprises most of the mass of our visible Universe, leading to worldwide experimental and observational efforts towards its discovery. A primary tool in this search is…

High Energy Physics - Experiment · Physics 2026-04-01 Yuan-Hann Chang , Cheng-Wei Chiang , Hien Thi Doan , Nick Houston , Jinmian Li , Tianjun Li , Lina Wu , Xin Zhang

The absence of a breakthrough in directly observing dark matter (DM) through prominent large-scale detectors motivates the development of novel tabletop experiments probing more exotic regions of the parameter space. If DM contains…

Instrumentation and Methods for Astrophysics · Physics 2025-01-20 M. Hirschel , V. Vadakkumbatt , N. P. Baker , F. M. Schweizer , J. C. Sankey , S. Singh , J. P. Davis

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

One of the most significant and practical figures of merit in axion haloscope searches is the scanning rate, because of the unknown axion mass. Under the best experimental parameters, the only way to improve the figure of merit is to…

Cosmology and Nongalactic Astrophysics · Physics 2021-05-19 S. Ahn , S. Lee , J. Choi , B. R. Ko , Y. K. Semertzidis

An axion-like particle (ALP) with mass $m_\phi \sim 10^{-15}$eV oscillates with frequency $\sim$1 Hz. This mass scale lies in an open window of astrophysical constraints, and appears naturally as a consequence of grand unification (GUT) in…

High Energy Physics - Phenomenology · Physics 2021-01-06 David J. E. Marsh , Wen Yin