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Observation Of A High-energy Cosmic-ray Family Caused By A Centauro-type Nuclear Interaction In The Joint Emulsion Chamber Experiment At The Pamirs
Authors
Amato N.M.
Amineva T.P.
+90 more
Aoki H.
Arata N.
Azimov S.A.
Azimov Z.A.
Bakhtigereev S.E.
Baradzei L.T.
Bellandi Filho J.
Bialobrzeska H.
Bielawska H.
Bobodjanov I.B.
Borisov A.S.
Cananov S.D.
Chadranyan L.Kh.
Cherdyntseva K.V.
Chinellato J.A.
Denisova V.G.
Dobrigkeit C.
Dobrotin N.A.
Dunaevsky A.M.
Emelyanov Yu.A.
Fauth A.C.
Fujimoto Y.
Funayama Y.
Gubar N.E.
Gulov Yu.A.
Guseva Z.M.
Hasegawa S.
Iljina N.P.
Ivanenko I.P.
Kanevskaya E.A.
Khalilov D.A.
Khisanishvilli L.A.
Krys A.
Kumano H.
Ladarija M.K.
Lattes C.M.G.
Lazareva T.V.
Leptukh G.G.
Linke M.
Maciaszszyk J.
Maldonado R.H.C.
Malinowski J.
Managadze A.K.
Maximenko V.M.
Menon M.J.
Mikhailova I.A.
Mukhamedshin R.A.
Mullajanov E.G.
Murzina E.A.
Myrtojieva Sh.
Nam R.A.
Navia O. C.E.
Nedel'ko O.E.
Nikolaeva L.P.
Normuradov F.
Nosov A.N.
Nowicka J.
Nuritdinov Kh.
Ohsawa A.
Oliveira Castro F.M.
Pomelova E.I.
Popova E.G.
Puchkov V.S.
Rakobolskaya I.V.
Roganova T.M.
Roinishvili N.N.
Ryabova N.G.
Sawayanagi K.
Semba H.
Shibata T.
Shibuya E.H.
Shoboronov Kh.
Slavatinsky S.A.
Smirnova M.D.
Smorodin Yu.A.
Svanidze M.S.
Sveshnikova L.G.
Tamada M.
Tomaszewski A.
Turtelli Jr. A.
Uryson A.V.
Wlodarczyk Z.
Yamashita S.
Yokoi K.
Yuldashbaev T.S.
Zaitseva E.G.
Zatsepin G.T.
Zelevinskaya N.G.
Zhdanov G.B.
Zimin M.V.
Publication date
26 November 2015
Publisher
'Elsevier BV'
Doi
Cite
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. © 1987.1901-2226233Bayburina, (1981) Nucl. Phys. B, 191, p. 1Lattes, Fujimoto, Hasegawa, Hadronic interactions of high energy cosmic-ray observed by emulsion chambers (1980) Physics Reports, 65, p. 151(1984) Trudy FIAN, 154, p. 1Borisov, (1984) Proc. Intern. Symp. on Cosmic rays and particle physics, p. 3. , TokyoRen, (1985) 19th Intern. Cosmic ray Conf., 6, p. 317. , La JollaYamashita, (1985) 19th Intern. Cosmic ray Conf., 6, p. 364. , La JollaTamada, (1977) Nuovo Cimento, 41 B, p. 245T. Shibata et al., to be publishedHillas, (1979) 16th Intern. Cosmic ray Conf., 6, p. 13. , KyotoBattiston, Measurement of the proton-antiproton elastic and total cross section at a centre-of-mass energy of 540 GeV (1982) Physics Letters B, 117, p. 126UA5 Collab., G.J. Alner et al., preprint CERN-EP/85-62Taylor, (1976) Phys. Rev. D, 14, p. 1217Burnett, (1984) Proc. Intern. Symp. on Cosmic rays and particle physics, p. 468. , Toky
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