Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/98245
Type: Artigo de periódico
Title: Observation Of A High-energy Cosmic-ray Family Caused By A Centauro-type Nuclear Interaction In The Joint Emulsion Chamber Experiment At The Pamirs
Author: Borisov A.S.
Cherdyntseva K.V.
Guseva Z.M.
Denisova V.G.
Dunaevsky A.M.
Kanevskaya E.A.
Maximenko V.M.
Nam R.A.
Puchkov V.S.
Slavatinsky S.A.
Smirnova M.D.
Smorodin Yu.A.
Uryson A.V.
Zelevinskaya N.G.
Zimin M.V.
Zhdanov G.B.
Mikhailova I.A.
Mukhamedshin R.A.
Nedel'ko O.E.
Nikolaeva L.P.
Zatsepin G.T.
Amineva T.P.
Baradzei L.T.
Ivanenko I.P.
Iljina N.P.
Lazareva T.V.
Managadze A.K.
Murzina E.A.
Pomelova E.I.
Popova E.G.
Rakobolskaya I.V.
Roganova T.M.
Ryabova N.G.
Sveshnikova L.G.
Cananov S.D.
Chadranyan L.Kh.
Khisanishvilli L.A.
Ladarija M.K.
Leptukh G.G.
Roinishvili N.N.
Svanidze M.S.
Azimov Z.A.
Bobodjanov I.B.
Gubar N.E.
Gulov Yu.A.
Normuradov F.
Shoboronov Kh.
Azimov S.A.
Khalilov D.A.
Myrtojieva Sh.
Mullajanov E.G.
Nosov A.N.
Nuritdinov Kh.
Yuldashbaev T.S.
Bakhtigereev S.E.
Dobrotin N.A.
Emelyanov Yu.A.
Zaitseva E.G.
Bielawska H.
Bialobrzeska H.
Linke M.
Malinowski J.
Maciaszszyk J.
Krys A.
Tomaszewski A.
Nowicka J.
Wlodarczyk Z.
Chinellato J.A.
Dobrigkeit C.
Bellandi Filho J.
Fauth A.C.
Lattes C.M.G.
Menon M.J.
Navia O. C.E.
Sawayanagi K.
Shibuya E.H.
Turtelli Jr. A.
Amato N.M.
Arata N.
Oliveira Castro F.M.
Maldonado R.H.C.
Aoki H.
Fujimoto Y.
Funayama Y.
Hasegawa S.
Kumano H.
Semba H.
Tamada M.
Yamashita S.
Shibata T.
Yokoi K.
Ohsawa A.
Abstract: An exotic cosmic-ray family event is observed in the large emulsion chamber exposed by the joint at the Pamirs (4360 m above sea level). The family is composed of 120γ-ray-induced showers and 37 hadron-induced showers with individual visible energy exceeding 1 TeV. The decisive feature of the event is the hadron dominance: ΣEγ, ΣE(γ) h, 〈Eγ, 〈E(γ) h〉, 〈Eγ·Rγ〉 and 〈E(γ)·Rh〉 being 298 TeV, 476 TeV, 2.5 TeV, 12.9 TeV, 28.6 GeV m and 173 GeV m, respectively. Most probably the event is due to a Centauro interaction, which occured in the atmosphere at ∼700 m above the chamber. The event will constitute the second beautiful candidate for a Centauro observed at the Pamirs. © 1987.
Editor: 
Rights: aberto
Identifier DOI: 10.1016/0370-2693(87)90871-9
Address: http://www.scopus.com/inward/record.url?eid=2-s2.0-0010950443&partnerID=40&md5=3f849f7556eb9566f54c211b4eb3626f
Date Issue: 1987
Appears in Collections:Unicamp - Artigos e Outros Documentos

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