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

Yi, Andrew K.; Ahn, Saebyeok; Kutlu, Çağlar; Kim, JinMyeong; Ko, B. R.; Ivanov, B. I.; Byun, HeeSu; Loo, Arjan F. van; Park, SeongTae; Jeong, J. H.; Kwon, Ohjoon; Nakamura, Y.; Uchaikin, S.; Choi, Jihoon; Lee, Soohyung; Lee, Myeong Jae; Shin, Yun Chang; Kim, Jinsu; Lee, Doyu; Ahn, Danho; Bae, Sungjae; Lee, Jiwon; Kim, Young-Geun; Gkika, Violeta; Lee, Ki Woong; Oh, Seonjeong; Seong, Taehyeon; Kim, Dong-Min; Chung, Woohyun; Matlashov, Andrei; Youn, S. W.; Semertzidis, Yannis K.

doi:10.1103/physrevlett.130.071002

Cited by 40 publications

(14 citation statements)

References 48 publications

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“…magnet was delayed by nearly a year due to the Covid-19 pandemic, but the commissioning run of CAPP-12TB was eventually carried out successfully in 2022, eight years after the inception of CAPP. During the experiment, a ULC operating in the 1.025−1.185 GHz range and a JPA optimized at 1.06−1.12 GHz were utilized, and axion data was received within the 1.09−1.11 GHz range [276]. The system noise was kept at 200 mK, the lowest among all axion experiments, resulting in a scanning rate of 1.4 MHz per day with DFSZ sensitivity.…”

Section: Ultra-light Cavity (Ulc) For 12tb Experimentsmentioning

confidence: 99%

“…In addition, the world's lowest level of system noise is achieved, less than 2 quanta, by use of powerful dilution refrigerator, advanced thermal engineering, and the Josephson parametric amplifier (JPA) from the collaborator -Nakamura group in Tokyo university. CAPP has searched axions around 1.1 GHz with 1 MHz/day of scan rate with DFSZ sensitivity for the case of 100% axions in the dark matter halo [276] and even for the case of 20% axions, CAPP will be soon available to search axions with more than a megahertz per day of scanning speed with DFSZ sensitivity with the potential for even faster scanning speeds if high temperature superconducting cavity technology is implemented.…”

Section: Introductionmentioning

confidence: 99%

“…Figure50: Summary of current bounds and prospects of ongoing and future searches for the axion-photon coupling. Regions shaded in colours correspond to experiments: mauve for laboratory[498,499,706,707,713,714,715] and collider[703,741,185,742,743,185,744,745,746,747,748,749,749,750,751] searches for axions, green for searches for solar axions[236,158], and blue for direct dark matter detection experiments[752,667,505,507,561,661,290,285,288,753,289,276,676,754,402,689,508,509,691,704,755,664,511,708, 677,…”

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confidence: 99%

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Feebly-interacting particles: FIPs 2020 workshop report

et al. 2021

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With the establishment and maturation of the experimental programs searching for new physics with sizeable couplings at the LHC, there is an increasing interest in the broader particle and astrophysics community for exploring the physics of light and feebly-interacting particles as a paradigm complementary to a New Physics sector at the TeV scale and beyond. FIPs 2020 has been the first workshop fully dedicated to the physics of feebly-interacting particles and was held virtually from 31 August to 4 September 2020. The workshop has gathered together experts from collider, beam dump, fixed target experiments, as well as from astrophysics, axions/ALPs searches, current/future neutrino experiments, and dark matter direct detection communities to discuss progress in experimental searches and underlying theory models for FIPs physics, and to enhance the cross-fertilisation across different fields. FIPs 2020 has been complemented by the topical workshop “Physics Beyond Colliders meets theory”, held at CERN from 7 June to 9 June 2020. This document presents the summary of the talks presented at the workshops and the outcome of the subsequent discussions held immediately after. It aims to provide a clear picture of this blooming field and proposes a few recommendations for the next round of experimental results.

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Section: Ultra-light Cavity (Ulc) For 12tb Experimentsmentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

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confidence: 99%

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Feebly-interacting particles: FIPs 2020 workshop report

et al. 2021

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“…To date, the most sensitive limits have been set by cavity haloscopes in mass ranges above 1 µeV/c 2 (240 MHz) [33][34][35]. When a microwave cavity is placed in a dc magnetic field, axions produce an effective current that runs along the magnetic field lines through the cavity.…”

Section: Introductionmentioning

confidence: 99%

Electromagnetic modeling and science reach of DMRadio-m$^3$

Collaboration¹,

AlShirawi²,

Bartram³

et al. 2023

Preprint

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DMRadio-m 3 is an experiment that is designed to be sensitive to KSVZ and DFSZ QCD axion models in the 10-200 MHz (41 neV/c 2 -0.83 µeV/c 2 ) range. The experiment uses a solenoidal dc magnetic field to convert an axion dark-matter signal to an ac electromagnetic response in a coaxial copper pickup. The current induced by this axion signal is measured by dc SQUIDs. In this work, we present the electromagnetic modeling of the response of the experiment to an axion signal over the full frequency range of DMRadio-m 3 , which extends from the low-frequency, lumped-element limit to a regime where the axion Compton wavelength is only a factor of two larger than the detector size. With these results, we determine the live time and sensitivity of the experiment. The primary science goal of sensitivity to DFSZ axions across 30-200 MHz can be achieved with a 3σ live scan time of 3.7 years.

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“…ivity [61]. However, several advances in various haloscope groups are being made in order to reach these models, where the axion is expected to be found with much more certainty according to the axion theory.…”

Section: Axionsmentioning

confidence: 99%

Development of resonant cavity-based microwave filters for axion detection

García-Barceló¹

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

Cited by 40 publications

References 48 publications

Feebly-interacting particles: FIPs 2020 workshop report

Feebly-interacting particles: FIPs 2020 workshop report

Electromagnetic modeling and science reach of DMRadio-m$^3$

Development of resonant cavity-based microwave filters for axion detection

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