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: Garraffo, Zulema Delia, Pignotti, Alberto
Publicado: 1973
Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05503213_v53_n2_p419_Garraffo
http://hdl.handle.net/20.500.12110/paper_05503213_v53_n2_p419_Garraffo
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spelling paper:paper_05503213_v53_n2_p419_Garraffo2023-06-08T15:41:17Z Hadronic scaling and ratios of cosmic-ray components in the atmosphere Garraffo, Zulema Delia Pignotti, Alberto 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. 1973 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05503213_v53_n2_p419_Garraffo 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.
author Garraffo, Zulema Delia
Pignotti, Alberto
spellingShingle Garraffo, Zulema Delia
Pignotti, Alberto
Hadronic scaling and ratios of cosmic-ray components in the atmosphere
author_facet Garraffo, Zulema Delia
Pignotti, Alberto
author_sort Garraffo, Zulema Delia
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
publishDate 1973
url https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_05503213_v53_n2_p419_Garraffo
http://hdl.handle.net/20.500.12110/paper_05503213_v53_n2_p419_Garraffo
work_keys_str_mv AT garraffozulemadelia hadronicscalingandratiosofcosmicraycomponentsintheatmosphere
AT pignottialberto hadronicscalingandratiosofcosmicraycomponentsintheatmosphere
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