Please use this identifier to cite or link to this item: https://physrep.ff.bg.ac.rs/handle/123456789/832
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dc.contributor.authorMaletić, D.en
dc.contributor.authorDragić, A.en
dc.contributor.authorBanjanac, R.en
dc.contributor.authorJoković, D.en
dc.contributor.authorVeselinović, N.en
dc.contributor.authorUdoviić, V.en
dc.contributor.authorSavić, M.en
dc.contributor.authorPuzović, Jovanen
dc.contributor.authorAniin, I.en
dc.date.accessioned2022-07-12T17:16:50Z-
dc.date.available2022-07-12T17:16:50Z-
dc.date.issued2013-01-01en
dc.identifier.issn1742-6588en
dc.identifier.urihttps://physrep.ff.bg.ac.rs/handle/123456789/832-
dc.description.abstractCosmic ray muons stopped in 5 cm thick plastic scintillators at surface and at depth of 25 m.w.e are studied. Apart from the stopped muon rate we measured the spectrum of muon decay electrons and the degree of polarization of stopped muons. Preliminary results for the Michel parameter yield values lower than the currently accepted one, while the asymmetry between the numbers of decay positrons registered in the upper and lower hemispheres appear higher than expected on the basis of numerous earlier studies.en
dc.relation.ispartofJournal of Physics: Conference Seriesen
dc.titleStopped cosmic-ray muons in plastic scintillators on the surface and at the depth of 25 m.w.een
dc.typeConference Paperen
dc.identifier.doi10.1088/1742-6596/409/1/012142en
dc.identifier.scopus2-s2.0-84874287973en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84874287973en
dc.relation.issue1en
dc.relation.volume409en
item.openairetypeConference Paper-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
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