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Cited by 916

The DOI matches its Crossref record; 13 of the 13 references it cites were found in a registry or an index.

Energy spectra of gamma rays, electrons, and neutrinos produced at proton-proton interactions in the very high energy regime

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Kelner, S. R., Aharonian, F. A., Bugayov, V. V.·2006·Physical Review D
DOI 10.1103/physrevd.74.034018
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Abstract

We present new parameterizations of energy spectra of secondary particles, $\ensuremath{\pi}$ mesons, gamma rays, electrons, and neutrinos produced in inelastic proton-proton collisions. The simple analytical approximations based on simulations of proton-proton interactions using the public available SIBYLL code provide very good accuracy for energy distributions of secondary products in the energy range above 100 GeV. Generally, the recommended analytical formulas deviate from the simulated distributions within a few percent over a large range of $x={E}_{i}/{E}_{p}$---the fraction of energy of the incident proton transferred to the secondaries. Finally, we describe an approximate procedure of continuation of calculations towards low energies, down to the threshold of $\ensuremath{\pi}$-meson production.

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Metadata

Authors
Kelner, S. R., Aharonian, F. A., & Bugayov, V. V.
Venue
Physical Review D
Publisher
American Physical Society (APS)
Published
2006-08-23
Volume
74
Issue
3
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
DOI
10.1103/physrevd.74.034018
OpenAlex
W2170070152
Cited by
916
References
13
FWCI
16.52
Type
journal article
Language
en
Open access
green

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