Experimental Search for Invisible Dark Matter Axions around 22μeV

Author:

Kim Younggeun1ORCID,Jeong Junu1ORCID,Youn SungWoo1ORCID,Bae Sungjae21ORCID,Lee Kiwoong1,van Loo Arjan F.34ORCID,Nakamura Yasunobu34ORCID,Oh Seonjeong1,Seong Taehyeon1ORCID,Uchaikin Sergey1ORCID,Kim Jihn E.5,Semertzidis Yannis K.12ORCID

Affiliation:

1. IBS

2. KAIST

3. RIKEN Center for Quantum Computing (RQC)

4. The University of Tokyo

5. Seoul National University

Abstract

The axion has emerged as the most attractive solution to two fundamental questions in modern physics related to the charge-parity invariance in strong interactions and the invisible matter component of our Universe. Over the past decade, there have been many theoretical efforts to constrain the axion mass based on various cosmological assumptions. Interestingly, different approaches from independent groups produce good overlap between 20 and 30μeV. We performed an experimental search to probe the presence of dark matter axions within this particular mass region. The experiment utilized a multicell cavity haloscope embedded in a 12 T magnetic field to seek for microwave signals induced by the axion-photon coupling. The results ruled out the KSVZ axions as dark matter over a mass range between 21.86 and 22.00μeV at a 90% confidence level. This represents a sensitive experimental search guided by specific theoretical predictions. Published by the American Physical Society 2024

Funder

Institute for Basic Science

Japan Society for the Promotion of Science

Korea National Science Foundation

Publisher

American Physical Society (APS)

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