Hadronic scaling and ratios of cosmic-ray components in the atmosphere
Using the scaling hypothesis of hadronic inclusive reactions at high energy and data from accelerators we compute ratios of cosmic-ray components in the atmosphere. For the μ+/μ- ratio at sea level we find that the inclusion on nuclear effects results in a better agreement with experimental data. In...
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| Autores principales: | , , |
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| Formato: | JOUR |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_05503213_v53_n2_p419_Garraffo |
| Aporte de: |
| Sumario: | Using the scaling hypothesis of hadronic inclusive reactions at high energy and data from accelerators we compute ratios of cosmic-ray components in the atmosphere. For the μ+/μ- ratio at sea level we find that the inclusion on nuclear effects results in a better agreement with experimental data. In the case of the (π+ + π-)/p ratio, we predict a value at high energy that is considerably larger than the one usually inferred from lower energy data. © 1973. |
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