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We propose a new method for detecting dark matter axions using a resonant cavity coupled with a quantum Hall system. When a small sample exhibiting quantum Hall effect is placed inside the cavity and the cavity is tuned to resonance,…

高能物理 - 唯象学 · 物理学 2026-04-24 Aiichi Iwazaki

A modification of the cavity technique for axion dark matter detection is described in which the cavity is driven with input power instead of being permeated by a static magnetic field. A small fraction of the input power is pumped by the…

高能物理 - 唯象学 · 物理学 2013-01-22 P. Sikivie

We estimate the synchrotron radiation of cosmic muons in a uniform magnetic field in the $\mu$eV-to-meV energy scale. Such events can potentially bring backgrounds to the axion dark matter searches. The GEANT4 software package is utilized…

仪器与探测器 · 物理学 2026-05-07 Dan Zhang , Gray Rybka , Edward J. Daw , Robyn Evren

The axion, as a leading dark matter candidate, is the target of many ongoing and proposed experimental searches based on its coupling to photons. Ultralight axions that couple to photons can also cause polarization rotation of light, which…

高能物理 - 唯象学 · 物理学 2024-10-08 Xucheng Gan , Lian-Tao Wang , Huangyu Xiao

Laboratory searches for ultralight axion dark matter (DM) have traditionally assumed the terrestrial density of axions is equal to the average density of DM in the solar system. However, quadratic couplings to matter introduce a non-trivial…

高能物理 - 唯象学 · 物理学 2026-02-25 Xiaofei Huang , Xiaolin Ma , Zitong Xu , Itay M. Bloch , Kai Wei

Dark matter induced event rate in an Earth-based detector is predicted to show an annual modulation as a result of the Earth's orbital motion around the Sun. We searched for this modulation signature using the ionization signal of the…

高能物理 - 实验 · 物理学 2024-11-25 50 Collaboration , P. Agnes , I. F. M. Albuquerque , T. Alexander , A. K. Alton , M. Ave , H. O. Back , G. Batignani , K. Biery , V. Bocci , W. M. Bonivento , B. Bottino , S. Bussino , M. Cadeddu , M. Cadoni , F. Calaprice , A. Caminata , M. D. Campos , N. Canci , M. Caravati , N. Cargioli , M. Cariello , M. Carlini , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Chashin , A. Chepurnov , C. Cicalò , G. Covone , D. D'Angelo , S. Davini , A. De Candia , S. De Cecco , G. De Filippis , G. De Rosa , A. V. Derbin , A. Devoto , M. D'Incecco , C. Dionisi , F. Dordei , M. Downing , D. D'Urso , M. Fairbairn , G. Fiorillo , D. Franco , F. Gabriele , C. Galbiati , C. Ghiano , C. Giganti , G. K. Giovanetti , A. M. Goretti , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Gulino , B. R. Hackett , K. Herner , T. Hessel , B. Hosseini , F. Hubaut , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , K. Keeter , C. L. Kendziora , M. Kimura , I. Kochanek , D. Korablev , G. Korga , A. Kubankin , M. Kuss , M. Kuźniak , M. La Commara , M. Lai , X. Li , M. Lissia , G. Longo , O. Lychagina , I. N. Machulin , L. P. Mapelli , S. M. Mari , J. Maricic , A. Messina , R. Milincic , J. Monroe , M. Morrocchi , X. Mougeot , V. N. Muratova , P. Musico , A. O. Nozdrina , A. Oleinik , F. Ortica , L. Pagani , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , K. Pelczar , N. Pelliccia , S. Piacentini , A. Pocar , D. M. Poehlmann , S. Pordes , S. S. Poudel , P. Pralavorio , D. D. Price , F. Ragusa , M. Razeti , A. Razeto , A. L. Renshaw , M. Rescigno , J. Rode , A. Romani , D. Sablone , O. Samoylov , E. Sandford , W. Sands , S. Sanfilippo , C. Savarese , B. Schlitzer , D. A. Semenov , A. Shchagin , A. Sheshukov , M. D. Skorokhvatov , O. Smirnov , A. Sotnikov , S. Stracka , Y. Suvorov , R. Tartaglia , G. Testera , A. Tonazzo , E. V. Unzhakov , A. Vishneva , R. B. Vogelaar , M. Wada , H. Wang , Y. Wang , S. Westerdale , M. M. Wojcik , X. Xiao , C. Yang , G. Zuzel

We report the first result of a direct search for a Cosmic ${\it axion}$ Background (C$a$B) - a relativistic background of axions that is not dark matter - performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX).…

Dark photons, as a minimal extension of the Standard Model through an additional Abelian gauge group, may propagate relativistically across the galaxy, originating from dark matter decay or annihilation, thereby contributing to a galactic…

Resonant feedback circuits are proposed as an alternative to normal modes of conducting wall cavities or lumped circuits in searches for hidden sector particles. The proposed method offers several potential advantages over the most…

仪器与探测器 · 物理学 2019-02-20 Edward J. Daw

We show that both the baryon asymmetry of the universe and dark matter (DM) can be accounted for by the dynamics of a single axion-like field. In this scenario, the observed baryon asymmetry is produced through spontaneous…

高能物理 - 唯象学 · 物理学 2019-02-13 Kyu Jung Bae , Jeff Kost , Chang Sub Shin

In this paper we study the effect of the channeling of ions recoiling from collisions with weakly interacting massive particles (WIMPs) in single crystal detectors. In particular we investigate the possibility that channeling may give rise…

天体物理仪器与方法 · 物理学 2015-05-19 Richard J. Creswick , Shmuel Nussinov , Frank T. Avignone

Mirror and more generic hidden sector dark matter models can simultaneously explain the DAMA, CoGeNT and CRESST dark matter signals consistently with the null results of the other experiments. This type of dark matter can be captured by the…

高能物理 - 唯象学 · 物理学 2015-05-30 R. Foot

An annual modulation signal due to the Earth orbiting around the Sun would be one of the strongest indications of the direct detection of dark matter. In 2016, we reported a search for dark matter by looking for this annual modulation with…

Axion-photon oscillation refers to the process of mutual conversion between photons and axions when they propagate in a magnetic field. This process depends on the strength of the background magnetic field, and magnetic white dwarfs provide…

高能物理 - 唯象学 · 物理学 2026-05-29 Hao-Chen Tian , Zhao-Yang Wang , Yun-Feng Liang , Zhao-Wei Du

Future multi-tonne Direct Detection experiments will be sensitive to solar neutrino induced nuclear recoils which form an irreducible background to light Dark Matter searches. Indeed for masses around 6 GeV the spectra of neutrinos and Dark…

高能物理 - 唯象学 · 物理学 2015-03-10 Jonathan H. Davis

Both axion and dark photon dark matter are among the most promising candidates of dark matter. What we know with some confidence is that they exhibit a small velocity distribution $\delta v\lesssim v\sim 10^{-3}$c. In addition, their mass…

高能物理 - 唯象学 · 物理学 2025-08-12 Puxian Wei , Ruifeng Zheng , Qiaoli Yang

We study the underlying theory of dielectric haloscopes, a new way to detect dark matter axions. When an interface between different dielectric media is inside a magnetic field, the oscillating axion field acts as a source of…

高能物理 - 唯象学 · 物理学 2017-02-01 Alexander J. Millar , Georg G. Raffelt , Javier Redondo , Frank D. Steffen

This study investigates the potential of the Sagnac Effect for detecting dark matter in the Solar System, particularly within the Sun. Originating from the relative delay and interference of light beams traveling in opposite directions on…

广义相对论与量子宇宙学 · 物理学 2024-12-03 A. D. S. Souza , C. R. Muniz , R. M. P. Neves , M. B. Cruz

We investigate the impact of the axionic coupling parameter on the bending angle of light and the shadow cast by slowly rotating black holes in Chern-Simons modified gravity. We utilize the Ishihara \etal method to derive the deflection…

广义相对论与量子宇宙学 · 物理学 2023-06-16 Nashiba Parbin , Dhruba Jyoti Gogoi , Umananda Dev Goswami

The orbit of the Earth about the Sun produces an annual modulation in the WIMP direct detection rate. If the local WIMP velocity distribution is isotropic then the modulation is roughly sinusoidal with maximum in June, however if the…

天体物理学 · 物理学 2014-10-13 Anne M Green