dc.creatorDuarte, L.
dc.creatorLin, L.
dc.creatorLindner, M.
dc.creatorKozhuharov, V.
dc.creatorKuleshov, S.V.
dc.creatorde Jesus, A.S.
dc.creatorQueiroz, F.S.
dc.creatorVillamizar, Y.
dc.creatorWestfahl, H., Jr.
dc.date.accessioned2023-09-11T15:50:34Z
dc.date.accessioned2024-05-02T15:12:04Z
dc.date.available2023-09-11T15:50:34Z
dc.date.available2024-05-02T15:12:04Z
dc.date.created2023-09-11T15:50:34Z
dc.date.issued2023-06
dc.identifierEuropean Physical Journal C Open Access Volume 83, Issue 6 June 2023 Article number 514
dc.identifier14346044
dc.identifierhttps://repositorio.unab.cl/xmlui/handle/ria/53118
dc.identifier10.1140/epjc/s10052-023-11603-x
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/9263731
dc.description.abstractWe propose the first Search for Dark Sector at the Brazilian Synchrotron Light Laboratory, site of Sirius, a fourth-generation storage ring. We show that UVX, Sirius predecessor, can be a promising dark sector detector, SeDS, with unprecedented sensitivity. The search is based on a 1 - 3 GeV positron beam impinging on a thick target leading the e+e-→ γA′ reaction, followed by a missing mass spectrum event reconstruction. We show that SeDS has the potential to probe dark photons with masses up to 55 MeV and kinetic coupling down to ϵ2∼ 10 - 12 . Therefore, such experiment would constitute the best dark photon probe worldwide in the 10 - 55 MeV mass range, being able to probe an unexplored region of parameter space.
dc.languageen
dc.publisherInstitute for Ionics
dc.rightshttps://creativecommons.org/licenses/by/4.0/
dc.rightsAttribution 4.0 International (CC BY 4.0)
dc.subjectDark Matter
dc.subjectMissing Mass (Astrophysics)
dc.subjectDarkness
dc.titleSearch for dark sector by repurposing the UVX Brazilian synchrotron
dc.typeArtículo


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