AAfrag 2.01: interpolation routines for Monte Carlo results on secondary production including light antinuclei in hadronic interactions

Kachelrieß, M.; Ostapchenko, S.; Tjemsland, J.

doi:10.1016/j.cpc.2023.108698

Cited by 3 publications

(1 citation statement)

References 35 publications

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“…Interestingly, the same proposed DM candidate (𝑚 𝜒 ≈ 50 − 100 GeV) can reproduce the 10 GeV antiproton excess, 𝛾-ray excess from thsce Galactic center, and the extended 𝛾-ray emission from the 400-kpc-across halo of the Andromeda galaxy (M31) [171,172] (see also references therein). Due to space limitations, I have to conclude my review with an incomplete list of papers that discuss astrophysical uncertainties associated with antiprotons [173][174][175][176][177][178][179], and the DM interpretation of the antiproton excess [180][181][182][183].…”

Section: Cosmic Ray Antiprotons and 10 Gev Excessmentioning

confidence: 99%

Direct measurements of cosmic rays and their possible interpretations

Moskalenko

2023

Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023)

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The last two decades have brought spectacular advances in astrophysics of cosmic rays (CRs) and space-and ground-based astronomy. Launches of missions that employ forefront detector technologies enabled measurements with large effective areas, wide fields of view, and precision that we recently could not even dream of. Meanwhile, interpretation of the individual slices of information about the internal working of the Milky Way provided by such experiments poses challenges to the traditional astrophysical models. New mysteries arise in the composition and spectra of CR species at low and high energies, in the energy range where we thought the main features were already understood fairly well. This accumulation of unsolved puzzles highlights the peculiarity of the current epoch and means that major breakthroughs are still ahead. In my talk, I review the current state of direct measurements of CRs and discuss their possible interpretations. Unfortunately, many important ideas and publications are not discussed here due to the space limitations.

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