Cited by 355Astrophysics and Cosmic PhenomenaParticle physics theoretical and experimental studiesHigh-Energy Particle Collisions Research

The DOI matches its Crossref record.

Parametrization of gamma-ray production cross sections forppinteractions in a broad proton energy range from the kinematic threshold to PeV energies

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Abstract

Using publicly available Monte Carlo codes as well as compilation of published data on $pp$ interactions for proton kinetic energy below 2 GeV, we parametrize the energy spectra and production rates of $\ensuremath{\gamma}$-rays by simple but quite accurate ($\ensuremath{\le}20%$) analytical expressions in a broad range from the kinematic threshold to PeV energies.

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Crossref · 10.1103/physrevd.90.123014

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  • At cosmic-ray proton energies ≲2 GeV, γ-ray production is primarily via resonant processes and through inverse Compton scattering of secondary leptonic particles.

    “At this energy, the γ -ray production is primarily via resonant processes (Kafexhiu et al. 2014) and through IC scattering of the secondary leptonic particles (equation 14) not included in the above equation.”

    From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Kafexhiu et al. 2014

  • Lower γ-ray production at cosmic-ray proton energies ≲2 GeV is expected due to the inefficiency of the inelastic collision as the proton energy reaches the rest mass energy of the proton.

    “The lower γ -ray production at Ep ≲ 2 GeV is expected due to the inefficiency of the inelastic collision as Ep reaches the rest mass energy of the proton.”

    From The Fermi/eROSITA bubbles: a look into the nuclear outflow from the Milky Way (2024) · cites this paper as Kafexhiu et al. 2014

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Metadata

Authors
Kafexhiu, E., Aharonian, F., Taylor, A. M., & Vila, G. S.
Affiliations
  • Max Planck Institute for Nuclear Physics (DE)
  • Dublin Institute For Advanced Studies (IE)
  • Consejo Nacional de Investigaciones Científicas y Técnicas (AR)
Venue
Physical Review D
Published
2014-12-29
Volume
90
Issue
12
ISSN
  • 0556-2821 (ISSN-L)
  • 1550-7998
  • 1550-2368
OpenAlex
W2093887493
Cited by
355
References
0
Citations by year
2026: 30 · 2025: 42 · 2024: 42 · 2023: 50 · 2022: 31 · 2021: 54 · 2020: 28 · 2019: 25 · 2018: 18 · 2017: 12 · 2016: 12 · 2015: 10 · 2014: 1
FWCI
5.14
Type
journal article
Language
en
Open access
Locations
  • Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields (publishedVersion)
  • arXiv (Cornell University) (publishedVersion)
  • Max Planck Digital Library (submittedVersion, other-oa)
  • MPG.PuRe (Max Planck Society) (submittedVersion, other-oa)
  • Conicet (submittedVersion, cc-by-nc-sa)
  • arXiv (Cornell University)
Funders
  • Dublin Institute for Advanced Studies
  • Consejo Nacional de Investigaciones Científicas y Técnicas
  • Agencia Nacional de Promoción Científica y Tecnológica (PIP 0078, PICT 2012-00278)
Topics
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Astrophysics and Cosmic Phenomena
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Particle physics theoretical and experimental studies
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › High-Energy Particle Collisions Research
Keywords
gamma-ray production cross sections, proton-proton collisions, parameterization, closed-form expressions, energy spectrum, production rate, kinematic threshold, cosmic rays, gamma-ray astronomy

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