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Air Shower Simulations in a Hybrid Approach using Cascade Equations

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arxiv astro-ph/0212018 v2 pith:QZ7X35PH submitted 2002-12-02 astro-ph

Air Shower Simulations in a Hybrid Approach using Cascade Equations

classification astro-ph
keywords showercascadeenergiesequationsapproachcarlohybridlateral
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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A new hybrid approach to air shower simulations is described. At highest energies, each particle is followed individually using the traditional Monte Carlo method; this initializes a system of cascade equations which are applicable for energies such that the shower is one-dimensional. The cascade equations are solved numerically down to energies at which lateral spreading becomes significant, then their output serves as a source function for a 3-dimensional Monte Carlo simulation of the final stage of the shower. This simulation procedure reproduces the natural fluctuations in the initial stages of the shower, gives accurate lateral distribution functions, and provides detailed information about all low energy particles on an event-by-event basis. It is quite efficient in computation time.

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  1. Measurement of charged-particle production in $\sqrt{s_\text{NN}}=9.62$ TeV proton-oxygen collisions as a probe of cosmic-ray air showers with the ATLAS detector

    hep-ex 2026-04 accept novelty 7.0

    ATLAS measured charged-particle production in 9.62 TeV p-O collisions, yielding a fiducial pO cross section of 396 mb and extrapolated p-air inelastic cross section of 406 mb, with distributions an order of magnitude ...