DC Field | Value | Language |
---|---|---|
dc.contributor.author | Chang, Seung Pyo | ko |
dc.contributor.author | Haciomeroglu, Selcuk | ko |
dc.contributor.author | Kim, On | ko |
dc.contributor.author | Lee, Soohyung | ko |
dc.contributor.author | Park, Seongtae | ko |
dc.contributor.author | Semertzidis, Yannis K. | ko |
dc.date.accessioned | 2023-07-05T08:00:37Z | - |
dc.date.available | 2023-07-05T08:00:37Z | - |
dc.date.created | 2023-06-08 | - |
dc.date.issued | 2017-10 | - |
dc.identifier.citation | 17th International Workshop on Polarized Sources, Targets and Polarimetry, PSTP 2017 | - |
dc.identifier.issn | 1824-8039 | - |
dc.identifier.uri | http://hdl.handle.net/10203/310323 | - |
dc.description.abstract | We 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.language | English | - |
dc.publisher | Sissa Medialab Srl | - |
dc.title | Axion dark matter search using the storage ring EDM method | - |
dc.type | Conference | - |
dc.identifier.scopusid | 2-s2.0-85073519013 | - |
dc.type.rims | CONF | - |
dc.citation.publicationname | 17th International Workshop on Polarized Sources, Targets and Polarimetry, PSTP 2017 | - |
dc.identifier.conferencecountry | KO | - |
dc.identifier.conferencelocation | Daejeon | - |
dc.contributor.localauthor | Semertzidis, Yannis K. | - |
dc.contributor.nonIdAuthor | Haciomeroglu, Selcuk | - |
dc.contributor.nonIdAuthor | Kim, On | - |
dc.contributor.nonIdAuthor | Lee, Soohyung | - |
dc.contributor.nonIdAuthor | Park, Seongtae | - |
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