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作 者:Marcus Bleicher
机构地区:[1]Institute for Theoretical Physics,Goethe-University Frankfurt,Max‑von‑Laue‑Str.1,60438 Frankfurt,Germany [2]Helmholtz Research Academy Hesse for FAIR(HFHF),GSI Helmholtzzentrum,Campus,Frankfurt,Germany
出 处:《Nuclear Science and Techniques》2024年第8期1-4,共4页核技术(英文)
摘 要:A new approach based on relativistic kinetic equations is proposed to solve the long-standing puzzle of light cluster formation, also called nucleosynthesis, in high-energy heavy-ion collisions. This method addresses the tension between STAR data and previous studies relying on either statistical equilibrium or coalescence approaches.
关 键 词:SYNTHESIS RELATIVISTIC CLUSTER
分 类 号:O571.6[理学—粒子物理与原子核物理]
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