Physics – High Energy Physics – High Energy Physics - Theory
Scientist
Physics
High Energy Physics
High Energy Physics - Theory
Scientist
Instituto de Física, Universidade Federal Fluminense, 24020-130 Niteroi, Rio de Janeiro, Brazil
Advanced Research Center for Science and Engineering, Waseda University, Shinjuku, Tokyo, 169 Japan
Instituto de Fisica Gleb Wataghin, Universidade Estadual de Campinas, Campinas, S.P.N. M.AmatoF. M. OliveiraCastroCentro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJR. H. C.MaldonadoInstitute de Fisica, Universidade Federal Fluminence, Niteroi, RJH.AokiY.FujimotoY.FunayamaS.HasegawaH.KumanoH.SembaT.TabukiM.TamadaK.TanakaS.YamashitaScience and Engineering Research Laboratory, Waseda University, Shinjuku, TokyoN.ArataT.ShibataK.YokoiDepartment of Physics, Aoyama Gakuin University, Setagaya, TokyoA.OhsawaInstitute for Cosmic-Ray Research, University of Tikyo, Tanashi, Tokyo
Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan
Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku, Tokyo, 169 Japan
Advanced Research Center for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, 169 Japan
Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, 169 Japan
Kyoto University, Japan; Bern, Universität, Switzerland
Instituto de Fisica Gleb Wataghin-Universidade Estadual de Campinas, Campinas, Sáo Paulo, BrasilN. M.AmatoF. M. OliveiraCastroCentro Brasileiro de Pesquisas Fisicas, Rio de Janeiro, RJ, BrasilH.AokiY.FujimotoS.HasegawaH.Kumanok.SawayanagiH.SembaT.TabukiM.TamadaS.YamashitaScience and Engineering Research Laboratory, Waseda University, Shinjuku, Tokyo, JapanN.ArataT.ShibataK.YokoiDepartment of Physics, Aoyama Gakuin University, Setagaya, Tokyo, JapanA.OhsawaInstitute for Cosmic Ray Research, Tokyo University, Tanashi, Tokyo, Japan
Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku, Tokyo 169, Japan
Nagoya University, Nagoya, Japan
Kinki Univ., Osaka, Japan.
A New Diagram Representing the Evolution of Galaxies
A new type of nuclear interactions in the ΣEγ>~1014 eV region
An Evolutional Track of Galaxies in L-(L/V) Diagram
Atmospheric Phenomena of High Energy Cosmic Rays at Mt. Chacaltaya. (Abstract)
Centauro and Mini Centauro
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