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    Deuteron, triton, helium-3, and hypertriton production in relativistic heavy-ion collisions via stochastic multiparticle reactions

    M. Ege1,2,*, J. Mohs1,2,†, J. Staudenmaier1,‡, and H. Elfner3,1,2,4,§

    • 1Institute for Theoretical Physics, Goethe University, Max-von-Laue-Strasse 1, 60438 Frankfurt am Main, Germany
    • 2Frankfurt Institute for Advanced Studies, Ruth-Moufang-Strasse 1, 60438 Frankfurt am Main, Germany
    • 3GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany
    • 4Helmholtz Research Academy Hesse for FAIR (HFHF), GSI Helmholtz Center, Campus Frankfurt, Max-von-Laue-Straße 12, 60438 Frankfurt am Main, Germany

    • *Contact author: mege@itp.uni-frankfurt.de
    • †Contact author: jmohs@itp.uni-frankfurt.de
    • ‡Left academia.
    • §Contact author: h.elfner@gsi.de

    Phys. Rev. C 112, 054908 – Published 25 November, 2025

    DOI: https://doi.org/10.1103/kppr-7zfv

    Abstract

    The production of light nuclei in heavy-ion collisions is an excellent probe for studying the phase diagram of quantum chromodynamics and for the search for a critical end point. In this work we apply a hybrid approach in which we study the light nuclei production in the afterburner stage of central Au+Au collisions at sNN=7.7, 14.5, and 19.6 GeV. In this stage, light nuclei are produced dynamically in 4↔2 catalysis reactions. A comparison of the dynamic production and a coalescence approach is presented for transverse momentum spectra of deuterons, tritons, He3 nuclei, and hypertritons and ratios of light nuclei yields. A good agreement with the experimentally measured yield of nuclei is found and we proceed to further investigate the production mechanisms of light nuclei by calculating the rates of the important channels for the formation and disintegration. We find that the afterburner stage is essential for the description of light nuclei formation in heavy-ion collisions, as light nuclei undergo a large number of interactions.

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