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액시온및극한상호작용연구단
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Search for Dark Matter Axions with Tunable TM020 Mode

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dc.contributor.authorSungjae Bae-
dc.contributor.authorJunu Jeong-
dc.contributor.authorYounggeun Kim-
dc.contributor.authorSung Woo Youn-
dc.contributor.authorHee Jun Park-
dc.contributor.authorTaehyeon Seong-
dc.contributor.authorSeonjeong Oh-
dc.contributor.authorYannis K. Semertzidis-
dc.date.accessioned2024-12-12T07:01:38Z-
dc.date.available2024-12-12T07:01:38Z-
dc.date.created2024-11-26-
dc.date.issued2024-11-
dc.identifier.issn0031-9007-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/15561-
dc.description.abstractAxions are hypothesized particles believed to potentially resolve two major puzzles in modern physics: the strong ⁢ problem and the nature of dark matter. Cavity-based axion haloscopes represent the most sensitive tools for probing their theoretically favored couplings to photons in the microelectronvolt range. However, as the search mass (or frequency) increases, the detection efficiency decreases, largely due to a decrease in cavity volume. Despite the potential of higher-order resonant modes to preserve experimental volume, their practical application in searches has been limited by the challenge of maintaining a high form factor over a reasonably wide search bandwidth. We introduce an innovative tuning method that uses the unique properties of auxetic materials, designed to effectively tune higher modes. This approach was applied to the TM020 mode for a dark matter axion search exploring a mass range from 21.38 to 21.79  μ⁢eV, resulting in the establishment of new exclusion limits for axion-photon coupling greater than approximately 10−13  GeV−1. These findings should allow use of higher-order modes for cavity haloscope searches.-
dc.language영어-
dc.publisherAmerican Physical Society-
dc.titleSearch for Dark Matter Axions with Tunable TM020 Mode-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.scopusid2-s2.0-85210978952-
dc.identifier.rimsid84537-
dc.contributor.affiliatedAuthorSungjae Bae-
dc.contributor.affiliatedAuthorJunu Jeong-
dc.contributor.affiliatedAuthorYounggeun Kim-
dc.contributor.affiliatedAuthorSung Woo Youn-
dc.contributor.affiliatedAuthorHee Jun Park-
dc.contributor.affiliatedAuthorTaehyeon Seong-
dc.contributor.affiliatedAuthorSeonjeong Oh-
dc.contributor.affiliatedAuthorYannis K. Semertzidis-
dc.identifier.doi10.1103/physrevlett.133.211803-
dc.identifier.bibliographicCitationPhysical Review Letters, v.133, no.21-
dc.relation.isPartOfPhysical Review Letters-
dc.citation.titlePhysical Review Letters-
dc.citation.volume133-
dc.citation.number21-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
Appears in Collections:
Center for Axion and Precision Physics Research(액시온 및 극한상호작용 연구단) > 1. Journal Papers (저널논문)
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