Abstract

AbstractThe production of deuterons and heavy clusters such as triton and helium (or even hypertriton) has gained increased attention during the last years. This attention was mainly stimulated by the recent hypertriton data and has led to the question of whether cluster production is driven by coalescence of its constituents or by thermal emission of the cluster itself. Here, we explore the cluster production by coalescence using the Ultra‐relativistic Quantum Molecular Dynamics model and a phase–space coalescence model. We explore deuteron production over a wide range of reactions and energies from GeV to TeV. Overall, we observe that coalescence leads to an excellent description of the deuteron yields and momentum distributions.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.