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Hill, C.T.; Schramm, D.N.
Fermi National Accelerator Lab., Batavia, IL (USA); Chicago Univ., IL (USA)1983
Fermi National Accelerator Lab., Batavia, IL (USA); Chicago Univ., IL (USA)1983
AbstractAbstract
[en] Ultra-high energy proton primaries interacting with the 30K photon background are treated as a transport phenomenon. Baryon number is explicitly conserved and the evolved spectrum develops a bump at a scale of order 5x1019 eV, below the cutoff, due to the pile-up of energy degraded protons. This may correspond in part to the observed ankle structure in the CR spectrum
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Source
Apr 1983; 4 p; 18. international cosmic ray conference; Bangalore (India); 22 Aug - 3 Sep 1983; CONF-830830--4; Available from NTIS, PC A02/MF A01 as DE83013711
Record Type
Report
Literature Type
Conference; Numerical Data
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