Observation of seasonal variation of atmospheric multiple-muon events in the NOvA Near Detector

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dc.creatorAcero Ortega, Mario A.
dc.creatorAdamson, P.
dc.creatorSoplin, Leonidas Aliaga
dc.creatorAlion, T.
dc.creatorAllakhverdian, Vladimir
dc.creatorAltakarli, Sef
dc.creatorAnfimov, Nikolay
dc.creatorAntoshkin, A.
dc.creatorAurisano, Adam
dc.creatorBack, A.
dc.creatorGomes, Ricardo Avelino
dc.date.accessioned2023-05-18T12:25:28Z
dc.date.available2023-05-18T12:25:28Z
dc.date.issued2019
dc.description.abstractUsing two years of data from the NOvA Near Detector at Fermilab, we report a seasonal variation of cosmic ray induced multiple-muon (Nμ ≥ 2) event rates which has an opposite phase to the seasonal variation in the atmospheric temperature. The strength of the seasonal multiple-muon variation is shown to increase as a function of the muon multiplicity. However, no significant dependence of the strength of the seasonal variation of the multiple-muon variation is seen as a function of the muon zenith angle, or the spatial or angular separation between the correlated muons.pt_BR
dc.identifier.citationACERO, M. A. et al. Observation of seasonal variation of atmospheric multiple-muon events in the NOvA Near Detector. Physical Review D, Washington, v. 99, n. 12, e122004, 2019. DOI: 10.1103/PhysRevD.99.122004. Disponível em: https://journals.aps.org/prd/pdf/10.1103/PhysRevD.99.122004. Acesso em: 16 maio 2023.pt_BR
dc.identifier.doi2470-0010
dc.identifier.doi10.1103/PhysRevD.99.122004
dc.identifier.issne- 2470-0029
dc.identifier.urihttp://repositorio.bc.ufg.br/handle/ri/22556
dc.language.isoengpt_BR
dc.publisher.countryEstados unidospt_BR
dc.publisher.departmentInstituto de Física - IF (RG)pt_BR
dc.rightsAcesso Abertopt_BR
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleObservation of seasonal variation of atmospheric multiple-muon events in the NOvA Near Detectorpt_BR
dc.typeArtigopt_BR

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