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Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model
The new scaling variable model explains the scaling behaviour of p+p to p+X inclusive reactions at CERN Intersecting Storage Ring energies. The cosmic antiproton spectrum has been derived from this model using the primary proton spectrum of Ryan et al. (1972). The derived antiproton-proton flux rati...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
1978
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/879092 |
_version_ | 1780908037594152960 |
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author | Bhattacharya, D P Basu, D Sarkar, K |
author_facet | Bhattacharya, D P Basu, D Sarkar, K |
author_sort | Bhattacharya, D P |
collection | CERN |
description | The new scaling variable model explains the scaling behaviour of p+p to p+X inclusive reactions at CERN Intersecting Storage Ring energies. The cosmic antiproton spectrum has been derived from this model using the primary proton spectrum of Ryan et al. (1972). The derived antiproton-proton flux ratio lies within the upper limit value of Bogomolov et al. (1971) and Chen (1972). (13 refs). |
id | cern-879092 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1978 |
record_format | invenio |
spelling | cern-8790922019-09-30T06:29:59Zhttp://cds.cern.ch/record/879092engBhattacharya, D PBasu, DSarkar, KCosmic antiproton spectrum at the top of the atmosphere derived from the new scaling modelAstrophysics and AstronomyThe new scaling variable model explains the scaling behaviour of p+p to p+X inclusive reactions at CERN Intersecting Storage Ring energies. The cosmic antiproton spectrum has been derived from this model using the primary proton spectrum of Ryan et al. (1972). The derived antiproton-proton flux ratio lies within the upper limit value of Bogomolov et al. (1971) and Chen (1972). (13 refs).oai:cds.cern.ch:8790921978 |
spellingShingle | Astrophysics and Astronomy Bhattacharya, D P Basu, D Sarkar, K Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
title | Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
title_full | Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
title_fullStr | Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
title_full_unstemmed | Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
title_short | Cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
title_sort | cosmic antiproton spectrum at the top of the atmosphere derived from the new scaling model |
topic | Astrophysics and Astronomy |
url | http://cds.cern.ch/record/879092 |
work_keys_str_mv | AT bhattacharyadp cosmicantiprotonspectrumatthetopoftheatmospherederivedfromthenewscalingmodel AT basud cosmicantiprotonspectrumatthetopoftheatmospherederivedfromthenewscalingmodel AT sarkark cosmicantiprotonspectrumatthetopoftheatmospherederivedfromthenewscalingmodel |