Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum

The recent CERN Intersecting Storage Ring cross section data on the p +p to pi /sup +or-/+X inclusive reactions have been analysed using the Bose-type distribution of the form E(d/sup 3/ sigma )/(d/sup 3/p)=(Axs /sup 1/2/)/(exp( epsilon ( lambda )/T)-1) proposed by Hoang (1973). This formula has bee...

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Detalles Bibliográficos
Autores principales: Bhattacharya, D P, Basu, D, Roychowdhury, R K
Lenguaje:eng
Publicado: 1976
Materias:
Particle Physics - Phenomenology
Acceso en línea:https://dx.doi.org/10.1088/0305-4616/2/9/015
http://cds.cern.ch/record/873998
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author Bhattacharya, D P
Basu, D
Roychowdhury, R K
author_facet Bhattacharya, D P
Basu, D
Roychowdhury, R K
author_sort Bhattacharya, D P
collection CERN
description The recent CERN Intersecting Storage Ring cross section data on the p +p to pi /sup +or-/+X inclusive reactions have been analysed using the Bose-type distribution of the form E(d/sup 3/ sigma )/(d/sup 3/p)=(Axs /sup 1/2/)/(exp( epsilon ( lambda )/T)-1) proposed by Hoang (1973). This formula has been used to derive the cosmic ray primary nucleon spectrum from the sea-level muon spectrum. It is found that the primary spectrum obeys the following relation: N(E/sub p/)dE/sub p /=2.06E/sub p//sup -2.64/dE/sub p/. The result has been compared with the recent experimental data and theoretical predictions given by different authors. (11 refs).
id cern-873998
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1976
record_format invenio
spelling cern-8739982019-09-30T06:29:59Zdoi:10.1088/0305-4616/2/9/015http://cds.cern.ch/record/873998engBhattacharya, D PBasu, DRoychowdhury, R KBose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrumParticle Physics - PhenomenologyThe recent CERN Intersecting Storage Ring cross section data on the p +p to pi /sup +or-/+X inclusive reactions have been analysed using the Bose-type distribution of the form E(d/sup 3/ sigma )/(d/sup 3/p)=(Axs /sup 1/2/)/(exp( epsilon ( lambda )/T)-1) proposed by Hoang (1973). This formula has been used to derive the cosmic ray primary nucleon spectrum from the sea-level muon spectrum. It is found that the primary spectrum obeys the following relation: N(E/sub p/)dE/sub p /=2.06E/sub p//sup -2.64/dE/sub p/. The result has been compared with the recent experimental data and theoretical predictions given by different authors. (11 refs).oai:cds.cern.ch:8739981976
spellingShingle Particle Physics - Phenomenology
Bhattacharya, D P
Basu, D
Roychowdhury, R K
Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
title Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
title_full Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
title_fullStr Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
title_full_unstemmed Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
title_short Bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
title_sort bose-type distribution and primary cosmic ray nucleon spectrum from sea-level muon spectrum
topic Particle Physics - Phenomenology
url https://dx.doi.org/10.1088/0305-4616/2/9/015
http://cds.cern.ch/record/873998
work_keys_str_mv AT bhattacharyadp bosetypedistributionandprimarycosmicraynucleonspectrumfromsealevelmuonspectrum
AT basud bosetypedistributionandprimarycosmicraynucleonspectrumfromsealevelmuonspectrum
AT roychowdhuryrk bosetypedistributionandprimarycosmicraynucleonspectrumfromsealevelmuonspectrum

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