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相关论文: High and low mass Axion Haloscopes at UWA

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We propose a variation, based on very low energy and extremely intense photon sources, on the well established technique of Light-Shining-through-Wall (LSW) experiments for axion-like particle searches. With radiation sources at 30 GHz, we…

高能物理 - 唯象学 · 物理学 2016-02-01 L. Capparelli , G. Cavoto , J. Ferretti , F. Giazotto , A. D. Polosa , P. Spagnolo

We discuss the physics case for and the concept of a medium-scale axion helioscope with sensitivities in the axion-photon coupling a few times better than CERN Axion Solar Telescope (CAST). Search for an axion-like particle with these…

We propose a new strategy to search for dark matter axions in the mass range of 40--400 $\mu$eV by introducing dielectric haloscopes, which consist of dielectric disks placed in a magnetic field. The changing dielectric media cause…

The goal of this paper is to introduce a novel likelihood-based inferential framework for axion haloscopes which is valid under the commonly applied "rescanning" protocol. The proposed method enjoys short data acquisition times and a simple…

数据分析、统计与概率 · 物理学 2023-07-19 Andrea Gallo Rosso , Sara Algeri , Jan Conrad

In an effort to extend the usefulness of microwave cavity detectors to higher axion masses, above ~8 $\mu$eV (~2 GHz), a numerical trade study of cavities was conducted to investigate the merit of using variable periodic post arrays and…

仪器与探测器 · 物理学 2016-03-24 I. Stern , A. A. Chisholm , J. Hoskins , P. Sikivie , N. S. Sullivan , D. B. Tanner , G. Carosi , K. van Bibber

We discuss the sensitivity of the present and near-future axion dark matter experiments to a halo of axions or axion-like particles gravitationally bound to the Earth or the Sun. The existence of such halos, assuming they are formed,…

高能物理 - 唯象学 · 物理学 2021-01-28 Abhishek Banerjee , Dmitry Budker , Joshua Eby , Victor V. Flambaum , Hyungjin Kim , Oleksii Matsedonskyi , Gilad Perez

The first part reviews the working mechanisms, capabilities and performance of axion helioscopes, including the achieved results so far. The 2nd part is observationally driven. New simulation results obtained with the Geant4 code…

太阳与恒星天体物理 · 物理学 2014-11-18 K. Zioutas , M. Tsagri , Y. Semertzidis , T. Papaevangelou , T. Dafni , V. Anastassopoulos

Haloscopes are resonant cavities that serve as detectors of dark matter axions when they are immersed in a strong static magnetic field. In order to increase the volume and improve its introduction within dipole or solenoid magnets for…

Axions are hypothetical particles that provide a compelling solution to two major mysteries in modern physics: the strong CP problem and the nature of dark matter. The plasma haloscope has been proposed as a promising approach for probing…

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…

仪器与探测器 · 物理学 2018-10-29 Ben T. McAllister , Maxim Goryachev , Jeremy Bourhill , Eugene N. Ivanov , Michael E. Tobar

To account for the dark matter content in our Universe, post-inflationary scenarios predict for the QCD axion a mass in the range $(10-10^3)\,\mu\mbox{eV}$. Searches with haloscope experiments in this mass range require the monitoring of…

The International Axion Observatory (IAXO) is a forth generation axion helioscope designed to detect solar axions and axion-like particles (ALPs) with a coupling to the photon $g_{a\gamma}$ down to a few $10^{-12}$ GeV$^{-1}$, 1.5 orders of…

仪器与探测器 · 物理学 2016-11-16 Maurizio Giannotti , Jaime Ruz , Julia K. Vogel

The CERN Axion Solar Telescope (CAST) experiment searches for solar axions by the "helioscope" method. First results imply an upper limit on the axion-photon coupling of g_a-gamma < 1.16 x 10^-10 GeV^-1 (95% CL) for m_a < 0.02 eV, in this…

高能物理 - 唯象学 · 物理学 2007-05-23 Georg G. Raffelt

A preliminary result of the solar axion search experiment at the University of Tokyo is presented. We searched for axions which could be produced in the solar core by exploiting the axion helioscope. The helioscope consists of a…

高能物理 - 实验 · 物理学 2009-10-31 Makoto Minowa , Shigetaka Moriyama , Yoshizumi Inoue , Toshio Namba , Yuko Takasu , Akira Yamamoto

We investigate the prospect of an alternative laboratory-based search for the coupling of axions and axion-like particles to photons. Here, the collision of two laser beams resonantly produces axions, and a signal photon is detected after…

高能物理 - 唯象学 · 物理学 2020-05-18 K. A. Beyer , G. Marocco , R. Bingham , G. Gregori

A brief review of particle physics motivations for axion existence is followed by a discussion of optical observables that can be used for axion detection. It is emphasised that the resonant photon - axion transition can occur in the…

高能物理 - 唯象学 · 物理学 2009-09-25 Ryszard Stroynowski , Ariel R. Zhitnitsky

The axion is a hypothetical elementary particle and cold dark matter candidate. In this RF cavity experiment, halo axions entering a resonant cavity immersed in a static magnetic field convert into microwave photons, with the resulting…

The axion is a highly motivated elementary particle which could address two fundamental questions in physics - the strong CP problem and the dark matter mystery. Experimental searches for this hypothetical particle have started to reach…

高能物理 - 唯象学 · 物理学 2021-10-28 Yannis K. Semertzidis , SungWoo Youn

This article aims at clarifying the situation about astrophysical sources that might be observed with haloscope experiments sensitive to gravitational waves in the 1-10 GHz band. The GrAHal setup is taken as a benchmark. We follow a very…

广义相对论与量子宇宙学 · 物理学 2025-03-13 Aurélien Barrau , Juan García-Bellido , Thierry Grenet , Killian Martineau

We have searched for solar axions with a detector which consists of a 4T x 2.3m superconducting magnet, PIN-photodiode X-ray detectors, and an altazimuth mount to track the sun. The conversion region is filled with cold helium gas which…

天体物理学 · 物理学 2011-04-11 Y. Inoue , M. Minowa , Y. Akimoto , R. Ota , T. Mizumoto , A. Yamamoto