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액시온및극한상호작용연구단
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Dark Matter Detection in the Stratosphere

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dc.contributor.authorCantatore, Giovanni-
dc.contributor.authorcetin, Serkant A.-
dc.contributor.authorFischer, Horst-
dc.contributor.authorFunk, Wolfgang-
dc.contributor.authorKaruza, Marin-
dc.contributor.authorKryemadhi, Abaz-
dc.contributor.authorMaroudas, Marios-
dc.contributor.authorOzbozduman, Kaan-
dc.contributor.authorYannis K. Semertzidis-
dc.contributor.authorZioutas, Konstantin-
dc.date.accessioned2023-07-24T22:01:14Z-
dc.date.available2023-07-24T22:01:14Z-
dc.date.created2023-07-17-
dc.date.issued2023-06-
dc.identifier.issn2073-8994-
dc.identifier.urihttps://pr.ibs.re.kr/handle/8788114/13621-
dc.description.abstractWe investigate the prospects for the direct detection of dark matter (DM) particles, incident on the upper atmosphere. A recent work relating the burst-like temperature excursions in the stratosphere at heights of & AP;38-47 km with low speed incident invisible streaming matter is the motivation behind this proposal. As an example, dark photons could match the reasoning presented in that work provided they constitute part of the local DM density. Dark photons emerge as a U(1) symmetry within extensions of the standard model. Dark photons mix with real photons with the same total energy without the need for an external field, as would be required, for instance, for axions. Furthermore, the ionospheric plasma column above the stratosphere can resonantly enhance the dark photon-to-photon conversion. Noticeably, the stratosphere is easily accessible with balloon flights. Balloon missions with up to a few tons of payload can be readily assembled to operate for months at such atmospheric heights. This proposal is not limited to streaming dark photons, as other DM constituents could be involved in the observed seasonal heating of the upper stratosphere. Therefore, we advocate a combination of different types of measurements within a multi-purpose parallel detector system, in order to increase the direct detection potential for invisible streaming constituents that affect, annually and around January, the upper stratosphere.-
dc.language영어-
dc.publisherMDPI-
dc.titleDark Matter Detection in the Stratosphere-
dc.typeArticle-
dc.type.rimsART-
dc.identifier.wosid001017937900001-
dc.identifier.scopusid2-s2.0-85163733555-
dc.identifier.rimsid81183-
dc.contributor.affiliatedAuthorYannis K. Semertzidis-
dc.identifier.doi10.3390/sym15061167-
dc.identifier.bibliographicCitationSYMMETRY-BASEL, v.15, no.6, pp.1 - 10-
dc.relation.isPartOfSYMMETRY-BASEL-
dc.citation.titleSYMMETRY-BASEL-
dc.citation.volume15-
dc.citation.number6-
dc.citation.startPage1-
dc.citation.endPage10-
dc.type.docTypeArticle-
dc.description.journalClass1-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscie-
dc.description.journalRegisteredClassscopus-
dc.relation.journalResearchAreaScience & Technology - Other Topics-
dc.relation.journalWebOfScienceCategoryMultidisciplinary Sciences-
dc.subject.keywordAuthorstreaming dark matter-
dc.subject.keywordAuthordirect detection-
dc.subject.keywordAuthorstratospheric anomaly-
Appears in Collections:
Center for Axion and Precision Physics Research(액시온 및 극한상호작용 연구단) > 1. Journal Papers (저널논문)
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