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Radio telescope search for the resonant conversion of cold dark matter axions from the magnetized astrophysical sources

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dc.contributor.authorFa Peng Huang-
dc.contributor.authorKenji Kadota-
dc.contributor.authorToyokazu Sekiguchi-
dc.contributor.authorHiroyuki Tashiro-
dc.date.available2018-12-13T10:46:13Z-
dc.date.created2018-07-23-
dc.date.issued2018-06-
dc.identifier.issn2470-0010-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/4973-
dc.description.abstractWe study the conditions for the adiabatic resonant conversion of the cold dark matter (CDM) axions into photons in the astrophysically sourced strong magnetic fields such as those in the neutron star magnetosphere. We demonstrate the possibility that the forthcoming radio telescopes such as the SKA (Square Kilometre Array) can probe those photon signals from the CDM axions. © 2018 authors. Published by the American Physical Society-
dc.language영어-
dc.publisherAMER PHYSICAL SOC-
dc.titleRadio telescope search for the resonant conversion of cold dark matter axions from the magnetized astrophysical sources-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.wosid000434630600002-
dc.identifier.scopusid2-s2.0-85049507533-
dc.identifier.rimsid64152-
dc.contributor.affiliatedAuthorFa Peng Huang-
dc.contributor.affiliatedAuthorKenji Kadota-
dc.identifier.doi10.1103/PhysRevD.97.123001-
dc.identifier.bibliographicCitationPhysical Review d, v.97, no.12, pp.1223001-
dc.relation.isPartOfPhysical Review d-
dc.citation.titlePhysical Review d-
dc.citation.volume97-
dc.citation.number12-
dc.citation.startPage1223001-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
Appears in Collections:
Center for Fundamental Theory(순수물리이론 연구단) > 1. Journal Papers (저널논문)
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Radio telescope search for the resonant conversion of cold dark matter axions from the magnetized astrophysical sources_Fa Peng Huang, Kenji Kadota.pdfDownload

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