% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@ARTICLE{Luoni:363848,
      author       = {Luoni, Francesca and Szabo, Reka and Boscolo, Daria and
                      Werneth, Charles},
      title        = {{GSI}-{ESA}-{NASA} {N}uclear {C}ross-section {D}atabase:
                      {U}pdate {I}. {A}ddition of {P}roton-projectile {R}eaction
                      {C}ross-sections},
      journal      = {Health physics},
      volume       = {130},
      number       = {2},
      issn         = {0017-9078},
      address      = {Baltimore, Md.},
      publisher    = {Lippincott Williams $\&$ Wilkins},
      reportid     = {GSI-2026-00054},
      pages        = {222 - 232},
      year         = {2026},
      abstract     = {Nuclear reaction cross-sections are needed for Monte Carlo
                      and deterministic radiation transport codes used for ion
                      therapy and radiation protection in space. A GSI-ESA-NASA
                      combined effort generated a free and publicly available
                      nucleus-nucleus reaction cross-section database.
                      Nevertheless, protons - the main component of solar particle
                      events and galactic cosmic ray fluences in space - account
                      alone for over $60\%$ of the effective dose behind thick
                      shields in space and are used in $88\%$ of the
                      cancer-treatment ion-therapy centers worldwide. Therefore,
                      in the present work, proton-projectile data have also been
                      included. These data are compared to the reaction
                      cross-section models used in radiation transport codes,
                      including the models of Tripathi-Cucinotta-Wilson,
                      Hybrid-Kurotama, Kox, Shen, and Kox-Shen. The
                      Tripathi-Cucinotta-Wilson model uses the Tripathi99 model
                      for low-Z projectile ions and the Tripathi96 model for other
                      projectiles. The Hybrid-Kurotama model is based on the Black
                      Sphere formula at high energies, which, for proton data, is
                      smoothly connected to the Tripathi99 model at low energies.
                      It is found that the Tripathi99 and Hybrid-Kurotama models
                      best fit the proton-projectile data.},
      keywords     = {Protons / Databases, Factual / Monte Carlo Method /
                      Radiation Protection: methods / United States / Cosmic
                      Radiation / Humans / ion therapy (Other) / nuclear reaction
                      cross-sections (Other) / proton-projectile cross-sections
                      (Other) / radiation protection in space (Other) / shielding
                      in space (Other) / space exploration (Other) / Protons (NLM
                      Chemicals)},
      cin          = {BIO},
      ddc          = {610},
      cid          = {I:(DE-Ds200)BIO-20160831OR354},
      pnm          = {633 - Life Sciences – Building Blocks of Life: Structure
                      and Function (POF4-633)},
      pid          = {G:(DE-HGF)POF4-633},
      experiment   = {$EXP:(DE-Ds200)no_experiment-20200803$},
      typ          = {PUB:(DE-HGF)16},
      doi          = {10.1097/HP.0000000000002055},
      url          = {https://repository.gsi.de/record/363848},
}