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:
- A.S. BorisovABA.S. Borisov
- K.V. CherdyntsevaKCK.V. Cherdyntseva
- Z.M. GusevaZGZ.M. Guseva
- V.G. DenisovaVDV.G. Denisova
- A.M. DunaevskyADA.M. Dunaevsky
- E.A. KanevskayaEKE.A. Kanevskaya
- V.M. MaximenkoVMV.M. Maximenko
- R.A. NamRNR.A. Nam
- V.S. PuchkovVPV.S. Puchkov
- S.A. SlavatinskySSS.A. Slavatinsky
- M D SmirnovaMSM D Smirnova
- Yu.A. SmorodinYSYu.A. Smorodin
- 1 May 1987
- journal article
- Published by Elsevier in Physics Letters B
- Vol. 190 (1-2) , 226-233
Abstract
No abstract availableKeywords
This publication has 5 references indexed in Scilit:
- Measurement of the proton-antiproton elastic and total cross section at a centre-of-mass energy of 540 GeVPhysics Letters B, 1982
- Nuclear interactions of super high energy cosmic-rays observed in mountain emulsion chambersNuclear Physics B, 1981
- Hadronic interactions of high energy cosmic-ray observed by emulsion chambersPhysics Reports, 1980
- Possible evidences in favour of a new type of cosmic-ray nuclear interaction named «centauro»Il Nuovo Cimento B (1971-1996), 1977
- Analysis of radial scaling in single-particle inclusive reactionsPhysical Review D, 1976