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...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autores principales: Garraffo, Z., Pignotti, A., Zgrablich, G.
Formato: JOUR
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_05503213_v53_n2_p419_Garraffo
Aporte de:
id todo:paper_05503213_v53_n2_p419_Garraffo
record_format dspace
spelling todo:paper_05503213_v53_n2_p419_Garraffo2023-10-03T15:34:16Z Hadronic scaling and ratios of cosmic-ray components in the atmosphere Garraffo, Z. Pignotti, A. Zgrablich, G. 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. Fil:Garraffo, Z. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. Fil:Pignotti, A. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales; Argentina. JOUR info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_05503213_v53_n2_p419_Garraffo
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
description 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.
format JOUR
author Garraffo, Z.
Pignotti, A.
Zgrablich, G.
spellingShingle Garraffo, Z.
Pignotti, A.
Zgrablich, G.
Hadronic scaling and ratios of cosmic-ray components in the atmosphere
author_facet Garraffo, Z.
Pignotti, A.
Zgrablich, G.
author_sort Garraffo, Z.
title Hadronic scaling and ratios of cosmic-ray components in the atmosphere
title_short Hadronic scaling and ratios of cosmic-ray components in the atmosphere
title_full Hadronic scaling and ratios of cosmic-ray components in the atmosphere
title_fullStr Hadronic scaling and ratios of cosmic-ray components in the atmosphere
title_full_unstemmed Hadronic scaling and ratios of cosmic-ray components in the atmosphere
title_sort hadronic scaling and ratios of cosmic-ray components in the atmosphere
url http://hdl.handle.net/20.500.12110/paper_05503213_v53_n2_p419_Garraffo
work_keys_str_mv AT garraffoz hadronicscalingandratiosofcosmicraycomponentsintheatmosphere
AT pignottia hadronicscalingandratiosofcosmicraycomponentsintheatmosphere
AT zgrablichg hadronicscalingandratiosofcosmicraycomponentsintheatmosphere
_version_ 1807321611608522752