9 research outputs found

    Concept of multiple-cell cavity for axion dark matter search

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    In cavity-based axion dark matter search experiments exploring high mass regions, multiple-cavity design is considered to increase the detection volume within a given magnet bore. We introduce a new idea, referred to as multiple-cell cavity, which provides various benefits including a larger detection volume, simpler experimental setup, and easier phase-matching mechanism. We present the characteristics of this concept and demonstrate the experimental feasibility with an example of a double-cell cavity.Comment: 8 pages, 11 figure

    Search for the Sagittarius Tidal Stream of Axion Dark Matter around 4.55 μ\mueV

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    We report the first search for the Sagittarius tidal stream of axion dark matter around 4.55 μ\mueV using CAPP-12TB haloscope data acquired in March of 2022. Our result excluded the Sagittarius tidal stream of Dine-Fischler-Srednicki-Zhitnitskii and Kim-Shifman-Vainshtein-Zakharov axion dark matter densities of ρa0.184\rho_a\gtrsim0.184 and 0.025\gtrsim0.025 GeV/cm3^{3}, respectively, over a mass range from 4.51 to 4.59 μ\mueV at a 90% confidence level.Comment: 6 pages, 7 Figures, PRD Letter accepte

    Development of an FPGA-based realtime DAQ system for axion haloscope experiments

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    A real-time Data Acquisition (DAQ) system for the CULTASK axion haloscope experiment was constructed and tested. The CULTASK is an experiment to search for cosmic axions using resonant cavities, to detect photons from axion conversion through the inverse Primakoff effect in a few GHz frequency range in a very high magnetic field and at an ultra low temperature. The constructed DAQ system utilizes a Field Programmable Gate Array (FPGA) for data processing and Fast Fourier Transformation. This design along with a custom Ethernet packet designed for real-time data transfer enables 100% DAQ efficiency, which is the key feature compared with a commercial spectrum analyzer. This DAQ system is optimally designed for RF signal detection in the axion experiment, with 100 Hz frequency resolution and 500 kHz analysis window. The noise level of the DAQ system averaged over 100,000 measurements is around -111.7 dBm. From a pseudo-data analysis, an improvement of the signal-to-noise ratio due to repeating and averaging the measurements using this real-time DAQ system was confirmed.11Nsciescopu

    Simulation study on optimization of cavity design for axion search experiments using COMSOL multiphysics

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    A conventional axion search experiment utilizes microwave resonant cavities, where axions are converted into photons under a strong magnetic field. Optimized cavity dimension is essential to enhance signal power from the axion-to-photon coupling, to broaden the frequency range, to minimize mode crossings, etc. An extensive study has been performed to optimize the dimension of a cavity and frequency tuning system using the COMSOL multiphysics simulation software. We introduce a figure of merit for this purpose, and present the results from the simulation study

    CAPP-8TB: Axion dark matter search experiment around 6.7 μev

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    © 2021 Elsevier B.V.CAPP-8TB is an axion dark matter search experiment dedicated to an axion mass search near 6.7μeV. The experiment uses a microwave resonant cavity under a strong magnetic field of 8T produced by a superconducting solenoid magnet in a dilution refrigerator. We describe the experimental configuration used to search for a mass range of 6.62 to 6.82μeV in the first phase of the experiment. We also discuss the next phase of the experiment and its prospects.11Nsciescopu

    Axion Dark Matter Search around 4.55 μeV with Dine-Fischler-Srednicki-Zhitnitskii Sensitivity

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    We report an axion dark matter search at Dine-Fischler-Srednicki-Zhitnitskii sensitivity with the CAPP-12TB haloscope, assuming axions contribute 100% of the local dark matter density. The search excluded the axion-photon coupling gaγγ down to about 6.2×10-16 GeV-1 over the axion mass range between 4.51 and 4.59 μeV at a 90% confidence level. The achieved experimental sensitivity can also exclude Kim-Shifman-Vainshtein-Zakharov axion dark matter that makes up just 13% of the local dark matter density. The CAPP-12TB haloscope will continue the search over a wide range of axion masses. © 2023 authors. Published by the American Physical Society.11Nsciescopu
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