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ISAI: Investigating Solar Axion by Iron-57

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arxiv 2212.13708 v1 pith:AH7ZCPT5 submitted 2022-12-28 astro-ph.IM astro-ph.GAhep-phphysics.ins-det

Tomonori Ikeda , Toshihiro Fujii , Takeshi Go Tsuru , Yuki Amano , Kazuho Kayama , Masamune Matsuda , Hiromu Iwasaki , Mizuki Uenomachi
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Kentaro Miuchi Yoshiyuki Onuki Yoshizumi Inoue Akimichi Taketa
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classification astro-ph.IMastro-ph.GAhep-phphysics.ins-det
keywords axionisaisolarinvestigatingiron-57x-rayapproachassociated
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The existence of the axion is a unique solution for the strong CP problem, and the axion is one of the most promising candidates of the dark matter. Investigating Solar Axion by Iron-57 (ISAI) is being prepared as a complemented table-top experiment to confirm the solar axion scenario. Probing an X-ray emission from the nuclear transitions associated with the axion-nucleon coupling is a leading approach. ISAI searches for the monochromatic 14.4 keV X-ray from the first excited state of 57Fe using a state-of-the-art pixelized silicon detector, dubbed XRPIX, under an extremely low-background environment. We highlight scientific objectives, experimental design and the latest status of ISAI.

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