Ultra high energy cosmic rays versus models of high energy hadronic interactions
Abstract We evaluate the consistency of hadronic interaction models in the CORSIKA simulation package with publicly available fluorescence telescope data from the Pierre Auger Observatory. By comparing the first few central moments of the extensive air shower depth maximum distributions, as extracte...
Saved in:
Main Authors: | Blaž Bortolato, Jernej F. Kamenik, Michele Tammaro |
---|---|
Format: | Article |
Language: | English |
Published: |
SpringerOpen
2025-02-01
|
Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-025-13861-3 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Resolution of (heavy) primaries in ultra high energy cosmic rays
by: Blaž Bortolato, et al.
Published: (2024-12-01) -
Ultra-High-Energy Cosmic Rays Accelerated by Magnetically Dominated Turbulence
by: Luca Comisso, et al.
Published: (2024-01-01) -
The Multimessenger Contribution of Ultra-High-Energy Cosmic Rays from Gamma-Ray Bursts
by: Zhenjiang Li, et al.
Published: (2025-01-01) -
Acceleration of Ultra-high-energy Cosmic Rays in the Kiloparsec-scale Jets of Nearby Radio Galaxies
by: Jie-Shuang Wang, et al.
Published: (2024-01-01) -
Combined Fit of Spectrum and Composition for FR0 Radio-galaxy-emitted Ultra–high energy Cosmic Rays with Resulting Secondary Photons and Neutrinos
by: Jon Paul Lundquist, et al.
Published: (2024-01-01)