The rapidity distribution of multiparticle production at the ISR and SppS collider energies are studied,and the data reveal a new empirical scaling behaviour in rapidity distributions in terms of the reduced variable....The rapidity distribution of multiparticle production at the ISR and SppS collider energies are studied,and the data reveal a new empirical scaling behaviour in rapidity distributions in terms of the reduced variable.Some relevant problems on the inclusive distribution of multiparticle productions are discussed.展开更多
Ⅰ. INTRODUCTION Owing to the rapid decrease of primary cosmic ray intensity with increasing energy, the detectors for recording super-high energy events must have very large acceptance. To study the super-high energy...Ⅰ. INTRODUCTION Owing to the rapid decrease of primary cosmic ray intensity with increasing energy, the detectors for recording super-high energy events must have very large acceptance. To study the super-high energy hadronic interaction at 1015—1017 eV, a large emulsion chamber with 150 m2 of sensitive area and one year’s sensitive time in one experimental period has been built on the top of Mt. Kanbala （5500 m a. s. 1.）展开更多
文摘The rapidity distribution of multiparticle production at the ISR and SppS collider energies are studied,and the data reveal a new empirical scaling behaviour in rapidity distributions in terms of the reduced variable.Some relevant problems on the inclusive distribution of multiparticle productions are discussed.
文摘Ⅰ. INTRODUCTION Owing to the rapid decrease of primary cosmic ray intensity with increasing energy, the detectors for recording super-high energy events must have very large acceptance. To study the super-high energy hadronic interaction at 1015—1017 eV, a large emulsion chamber with 150 m2 of sensitive area and one year’s sensitive time in one experimental period has been built on the top of Mt. Kanbala （5500 m a. s. 1.）
