Axion dark matter search using the storage ring EDM method

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dc.contributor.authorChang, Seung Pyoko
dc.contributor.authorHaciomeroglu, Selcukko
dc.contributor.authorKim, Onko
dc.contributor.authorLee, Soohyungko
dc.contributor.authorPark, Seongtaeko
dc.contributor.authorSemertzidis, Yannis K.ko
dc.date.accessioned2023-07-05T08:00:37Z-
dc.date.available2023-07-05T08:00:37Z-
dc.date.created2023-06-08-
dc.date.issued2017-10-
dc.identifier.citation17th International Workshop on Polarized Sources, Targets and Polarimetry, PSTP 2017-
dc.identifier.issn1824-8039-
dc.identifier.urihttp://hdl.handle.net/10203/310323-
dc.description.abstractWe propose using a modified storage ring EDM method to search for the axion dark matter induced EDM oscillation in nucleons. The method uses a combination of B and E-fields to produce a resonance between the g − 2 precession frequency and the background axion field oscillation to greatly enhance the sensitivity to it. An axion frequency range of 10−9 Hz to 100 MHz can be scanned with high sensitivity, corresponding to fa range of 1013 GeV ≤ fa ≤ 1030 GeV the breakdown scale of the global symmetry generating the axion or axion like particles (ALPs).-
dc.languageEnglish-
dc.publisherSissa Medialab Srl-
dc.titleAxion dark matter search using the storage ring EDM method-
dc.typeConference-
dc.identifier.scopusid2-s2.0-85073519013-
dc.type.rimsCONF-
dc.citation.publicationname17th International Workshop on Polarized Sources, Targets and Polarimetry, PSTP 2017-
dc.identifier.conferencecountryKO-
dc.identifier.conferencelocationDaejeon-
dc.contributor.localauthorSemertzidis, Yannis K.-
dc.contributor.nonIdAuthorHaciomeroglu, Selcuk-
dc.contributor.nonIdAuthorKim, On-
dc.contributor.nonIdAuthorLee, Soohyung-
dc.contributor.nonIdAuthorPark, Seongtae-
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PH-Conference Papers(학술회의논문)
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