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
Open accessAbstract
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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Cites
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Production and Propagation of Cosmic‐Ray Positrons and Electrons
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Diffuse Continuum Gamma Rays from the Galaxy
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Quark-gluon-string model and EAS simulation problems at ultra-high energies
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Can diffusive shock acceleration in supernova remnants account for high-energy galactic cosmic rays?
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sibyll: An event generator for simulation of high energy cosmic ray cascades
Fletcher, R. S., Gaisser, T. K., Lipari, P., & Stanev, T. (1994) · Physical Review D · doi:10.1103/physrevd.50.5710 · Cited by 409
Lepton spectra in the earth's atmosphere
Lipari, P. (1993) · Astroparticle Physics · doi:10.1016/0927-6505(93)90022-6 · Cited by 355
The Galactic Diffuse Gamma‐Ray Spectrum from Cosmic‐Ray Proton Interactions
Mori, M. (1997) · The Astrophysical Journal · doi:10.1086/303785 · Cited by 117
Production spectrum of gamma rays in interstellar space through neutral pion decay
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Parametrizations of inclusive cross sections for pion production in proton-proton collisions
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Expected neutrino signal from supernova remnant RX J1713.7-3946 and flavor oscillations
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Cited by
Kafexhiu, E., Aharonian, F., Taylor, A. M., & Vila, G. S. (2014) · Physical Review D · doi:10.1103/physrevd.90.123014 · Cited by 355
Self-citationGalactic halo origin of the neutrinos detected by IceCube
Taylor, A. M., Gabici, S., & Aharonian, F. (2014) · Physical Review D · doi:10.1103/physrevd.89.103003 · Cited by 113
Self-citationThe Fermi bubbles: gamma-ray, microwave and polarization signatures of leptonic AGN jets
Yang, H.-Y. K., Ruszkowski, M., & Zweibel, E. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1772 · Cited by 70
High Energy Neutrinos from the Fermi Bubbles
Lunardini, C., & Razzaque, S. (2012) · Physical Review Letters · doi:10.1103/physrevlett.108.221102 · Cited by 31
FERMI BUBBLE γ-RAYS AS A RESULT OF DIFFUSIVE INJECTION OF GALACTIC COSMIC RAYS
Thoudam, S. (2013) · The Astrophysical Journal · doi:10.1088/2041-8205/778/1/l20 · Cited by 24
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
- OpenAlex
- W2170070152
- Cited by
- 916
- References
- 13
- FWCI
- 16.52
- Type
- journal article
- Language
- en
- Open access
- green
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