Production of Energetic Light Fragments in CEM, LAQGSM, and MCNP6
Stepan G. Mashnik, Leslie M. Kerby, Konstantin K. Gudima, Arnold J., Sierk, Jeffrey S. Bull, and Michael R. James

TL;DR
This paper enhances the CEM, LAQGSM, and MCNP6 models to better simulate energetic light fragment production in nuclear reactions up to 1 TeV/nucleon, improving their predictive accuracy and applicability.
Contribution
The authors extend and modify existing nuclear reaction models to include production of heavier light fragments and improve spectral calculations, with validation against experimental data.
Findings
Enhanced models accurately reproduce experimental light fragment spectra.
Increased predictive power for reactions involving heavy light fragments.
Models now simulate a broader range of nuclear reactions with improved reliability.
Abstract
We extend the cascade-exciton model (CEM), and the Los Alamos version of the quark-gluon string model (LAQGSM), event generators of the Monte-Carlo N-particle transport code version 6 (MCNP6), to describe production of energetic light fragments (LF) heavier than 4He from various nuclear reactions induced by particles and nuclei at energies up to about 1 TeV/nucleon. In these models, energetic LF can be produced via Fermi break-up, preequilibrium emission, and coalescence of cascade particles. Initially, we study several variations of the Fermi break-up model and choose the best option for these models. Then, we extend the modified exciton model (MEM) used by these codes to account for a possibility of multiple emission of up to 66 types of particles and LF (up to 28Mg) at the preequilibrium stage of reactions. Then, we expand the coalescence model to allow coalescence of LF from…
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