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Secondary neutral pion-nucleon flux ratio at the top of the atmosphere
The CERN Intersecting Storage Ring data on the inclusive reaction p+p to pi /sup 0/+X has been fitted with a phenomenological form E(d/sup 3 / sigma /d/sup 3/p)=f(x, p/sub T/)=W/sub c/(a, b, z), where W/sub c /(a, b, z) is the generalised confluent function defined by W/sub c /(a, b, z)=e/sup -cz/ M...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1979
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Materias: | |
Acceso en línea: | http://cds.cern.ch/record/875290 |
_version_ | 1780907803958837248 |
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author | Roychoudhury, R K Bhattacharya, D P |
author_facet | Roychoudhury, R K Bhattacharya, D P |
author_sort | Roychoudhury, R K |
collection | CERN |
description | The CERN Intersecting Storage Ring data on the inclusive reaction p+p to pi /sup 0/+X has been fitted with a phenomenological form E(d/sup 3 / sigma /d/sup 3/p)=f(x, p/sub T/)=W/sub c/(a, b, z), where W/sub c /(a, b, z) is the generalised confluent function defined by W/sub c /(a, b, z)=e/sup -cz/ M(a, b, z). M(a, b, z) being the well known Kummer's function. Using this form and the primary proton spectrum of the Goddard Space Flight Center group the secondary neutral pion- nucleon flux ratio at the top of the atmosphere has been estimated. The derived result has been compared with those expected from p+p to pi /sup +or-/+X data, via different models. (8 refs). |
id | cern-875290 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1979 |
record_format | invenio |
spelling | cern-8752902019-09-30T06:29:59Zhttp://cds.cern.ch/record/875290engRoychoudhury, R KBhattacharya, D PSecondary neutral pion-nucleon flux ratio at the top of the atmosphereParticle Physics - PhenomenologyThe CERN Intersecting Storage Ring data on the inclusive reaction p+p to pi /sup 0/+X has been fitted with a phenomenological form E(d/sup 3 / sigma /d/sup 3/p)=f(x, p/sub T/)=W/sub c/(a, b, z), where W/sub c /(a, b, z) is the generalised confluent function defined by W/sub c /(a, b, z)=e/sup -cz/ M(a, b, z). M(a, b, z) being the well known Kummer's function. Using this form and the primary proton spectrum of the Goddard Space Flight Center group the secondary neutral pion- nucleon flux ratio at the top of the atmosphere has been estimated. The derived result has been compared with those expected from p+p to pi /sup +or-/+X data, via different models. (8 refs).oai:cds.cern.ch:8752901979 |
spellingShingle | Particle Physics - Phenomenology Roychoudhury, R K Bhattacharya, D P Secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
title | Secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
title_full | Secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
title_fullStr | Secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
title_full_unstemmed | Secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
title_short | Secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
title_sort | secondary neutral pion-nucleon flux ratio at the top of the atmosphere |
topic | Particle Physics - Phenomenology |
url | http://cds.cern.ch/record/875290 |
work_keys_str_mv | AT roychoudhuryrk secondaryneutralpionnucleonfluxratioatthetopoftheatmosphere AT bhattacharyadp secondaryneutralpionnucleonfluxratioatthetopoftheatmosphere |