Extensive Search for Axion Dark Matter over 1 GHz with CAPP’S Main Axion Experiment
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 frequency (mass) range of 1.025 GHz (<a:math xmlns:a="http://www.w3.org/1998/Math/MathML" display="inline"><a:mrow><a:mn>4.24</a:mn><a:mtext> </a:mtext><a:mtext> </a:mtext><a:mi mathvariant="normal">μ</a:mi><a:mi>eV</a:mi></a:mrow></a:math>) to 1.185 GHz (<d:math xmlns:d="http://www.w3.org/1998/Math/MathML" display="inline"><d:mrow><d:mn>4.91</d:mn><d:mtext> </d:mtext><d:mtext> </d:mtext><d:mi mathvariant="normal">μ</d:mi><d:mi>eV</d:mi></d:mrow></d:math>). We have introduced a number of innovations in this field, demonstrating the practical approach of optimizing all the relevant parameters of axion haloscopes, extending presently available technology. The CAPP 12 T magnet with an aperture of 320 mm made of <g:math xmlns:g="http://www.w3.org/1998/Math/MathML" display="inline"><g:mrow><g:msub><g:mrow><g:mi>Nb</g:mi></g:mrow><g:mrow><g:mn>3</g:mn></g:mrow></g:msub><g:mi>Sn</g:mi></g:mrow></g:math> and NbTi superconductors surrounding a 37 l ultralight-weight copper cavity is expected to convert Dine-Fischler-Srednicki-Zhitnitsky axions into approximately <i:math xmlns:i="http://www.w3.org/1998/Math/MathML" display="inline"><i:msup><i:mn>10</i:mn><i:mn>2</i:mn></i:msup></i:math> microwave photons per second. A powerful dilution refrigerator, capable of keeping the core system below 40 mK, combined with quantum-noise-limited readout electronics, achieved a total system noise of about 200 mK or below, which corresponds to a background of roughly <k:math xmlns:k="http://www.w3.org/1998/Math/MathML" display="inline"><k:mn>4</k:mn><k:mo>×</k:mo><k:msup><k:mn>10</k:mn><k:mn>3</k:mn></k:msup></k:math> photons per second within the axion bandwidth. The combination of all those improvements provides unprecedented search performance, imposing the most stringent exclusion limits on axion-photon coupling in this frequency range to date. These results also suggest an experimental capability suitable for highly sensitive searches for axion dark matter above 1 GHz. Published by the American Physical Society 2024
Authors
- B. R. Ko (ORCID: https://orcid.org/0000-0002-4591-5269)
- Andrew K. Yi (ORCID: https://orcid.org/0009-0001-8822-3844)
- Yun Chang Shin (ORCID: https://orcid.org/0000-0002-4997-0214)
- Hyoungsoon Choi (ORCID: https://orcid.org/0000-0002-7290-4362)
- Jihn E. Kim
- Violeta Gkika
- Pallavi Parashar
- Jihoon Choi (ORCID: https://orcid.org/0000-0003-2162-8895)
- Yasunobu Nakamura (ORCID: https://orcid.org/0000-0003-0424-630X)
- B. I. Ivanov (ORCID: https://orcid.org/0000-0003-3410-349X)
- L. Miceli (ORCID: https://orcid.org/0000-0001-8172-3769)
- S. Uchaikin (ORCID: https://orcid.org/0000-0003-2955-3306)
- Yonuk Chong (ORCID: https://orcid.org/0000-0002-6677-7109)
- Saebyeok Ahn (ORCID: https://orcid.org/0000-0001-9354-9083)
- SungWoo Youn (ORCID: https://orcid.org/0000-0003-4956-9372)
- Arjan F. van Loo (ORCID: https://orcid.org/0000-0001-8038-3088)
- M. J. Lee (ORCID: https://orcid.org/0000-0003-4528-4601)
- Ki Woong Lee
- HeeSu Byun
- Woohyun Chung (ORCID: https://orcid.org/0000-0002-6786-8176)
- J. H. Jeong (ORCID: https://orcid.org/0000-0003-0194-9587)
- Doyu Lee (ORCID: https://orcid.org/0000-0003-4129-4837)
- Sungjae Bae (ORCID: https://orcid.org/0000-0001-5116-2016)
- Andrei Matlashov (ORCID: https://orcid.org/0000-0002-3917-9891)
- Ohjoon Kwon (ORCID: https://orcid.org/0000-0002-7617-2509)
- JinMyeong Kim (ORCID: https://orcid.org/0000-0003-2153-2148)
- Danho Ahn (ORCID: https://orcid.org/0000-0003-2224-9467)
- Yannis K. Semertzidis (ORCID: https://orcid.org/0000-0001-7941-6639)
- Çağlar Kutlu (ORCID: https://orcid.org/0000-0002-8942-8550)
- SeongTae Park
- Soohyung Lee (ORCID: https://orcid.org/0000-0001-5959-9407)
- Taehyeon Seong (ORCID: https://orcid.org/0000-0003-3409-2815)
- Jiwon Lee (ORCID: https://orcid.org/0000-0001-6621-646X)
- Jinsu Kim (ORCID: https://orcid.org/0000-0002-6739-2833)
- Seonjeong Oh (ORCID: https://orcid.org/0009-0009-5883-735X)
- Young-Geun Kim (ORCID: https://orcid.org/0000-0001-7297-8110)
Institutions
- Seoul National University (KR)
- Korea Advanced Institute of Science and Technology (KR)
- Institute for Basic Science (KR)
- Computing Center (RU)
- RIKEN Center for Quantum Computing
- The University of Tokyo (JP)
Publication Details
- Journal
- Physical Review X
- Published
- 2024-08-12
- DOI
- https://doi.org/10.1103/physrevx.14.031023
- Citations
- 39
- Primary Topic
- Dark Matter and Cosmic Phenomena
- Type
- article
- Field-Weighted Citation Impact
- 25.73
Funders
- Institute for Basic Science
- Japan Society for the Promotion of Science