Study of low energy hadronic interaction models based on BESS observed cosmic ray proton and antiproton spectra at medium high altitude

Journal Article · Mon Jun 01 00:00:00 EDT 2009 · Physical Review. D, Particles Fields

DOI:https://doi.org/10.1103/PHYSREVD.79.114027· OSTI ID:21300860

Bhadra, Arunava; Mukherjee, Arindam ^[1]; Ghosh, Sanjay K; Raha, Sibaji ^[2]; Joarder, Partha S ^[3]

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1. High Energy and Cosmic Ray Research Centre, University of North Bengal, Siliguri, West Bengal, 734013 (India)
2. Department of Physics, Bose Institute, 93/1 A.P.C. Road, Kolkata, 700009 (India)
3. Centre for Astroparticle Physics and Space Science, Bose Institute, Block EN, Sector V, Salt Lake, Kolkata, 700091 (India)

We study low energy hadronic interaction models based on BESS observed cosmic ray proton and antiproton spectra at medium high altitude. Among the three popular low energy interaction models, we find that FLUKA reproduces the results of BESS observations on the secondary proton spectrum reasonably well over the whole observed energy range, the model UrQMD works well at relatively higher energies, whereas the spectrum obtained with GHEISHA differs significantly from the measured spectrum. The simulated antiproton spectrum with FLUKA, however, exhibits significant deviation from the BESS observation whereas UrQMD and GHEISHA reproduce the BESS observations within experimental error.

• OSTI ID: 21300860
• Journal Information: Physical Review. D, Particles Fields, Vol. 79, Issue 11; Other Information: DOI: 10.1103/PhysRevD.79.114027; (c) 2009 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); ISSN 0556-2821
• Country of Publication: United States
• Language: English

Related Subjects

72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
ANTIPROTONS
COSMIC RADIATION
ENERGY RANGE
INTERACTIONS
PROTON SPECTRA
SIMULATION