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Charge ratio of cosmic pions in the atmosphere

D. P. Bhattacharyya ; Indian Association for the Cultivation of Science, Jadavpur, Calcutta
R. K. Roychoudhury ; Indian Association for the Cultivation of Science, Jadavpur, Calcutta
Kalpana Sarkar ; Indian Association for the Cultivation of Science, Jadavpur, Calcutta

Sažetak

It is found that the CERN Intersecting Storage Ring data on pp => π± + X inclusive reactions can be represented by a single scaling variable η = 2p2Tx/(c ln(s/s0)) for 0.075 ≤ x ≤ 0.3 and 0.2 ≤ pT ≤ 1.5 GeV/c. The charge ratio of cosmic pion spectrum at the top of the atmosphere has been estimated using this new type of scaling variable and the primary nucleon spectrum of Grigorov et al. has been used as a hadron source at the top of the atmosphere.

Ključne riječi

Hrčak ID:

323227

URI

https://hrcak.srce.hr/323227

Datum izdavanja:

28.11.1977.

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