PSI Paul Scherrer Institut’s Post

🌟 🌠 The synthesis of elements heavier than iron within stars typically aligns well with theoretical models—except for one puzzling outlier: cerium-140. An international team of scientists, including researchers from PSI, has conducted groundbreaking experiments at CERN'sneutron time-of-flight (n_TOF) facility, yielding results that could challenge current understanding. 💬 "We might need to completely rethink the theoretical model for how elements heavier than iron are formed inside stars," says Emilio Maugeri from PSI's Laboratory for Radiochemistry. The formation of these heavy elements is primarily governed by two processes: the slow (s) and rapid (r) neutron capture processes. The s-process, in particular, has been accurately modeled, matching the observed abundance of these elements in certain stars within the Milky Way. ⭐ However, in some stars, where cerium-140 is produced via the s-process, astrophysicists have observed a significantly higher abundance of this isotope than predicted. If both the measurements and the model are correct, an unknown mechanism must account for this discrepancy. 🤔 Physicists have long theorized a potential third process, the intermediate (i) process, which might explain these findings. Emilio Andrea Maugeri is excited: "We may have just opened up an entirely new field of research." Next year, experts plan to convene at a dedicated conference to discuss the next steps forward. Read the full story here: https://brnw.ch/21wM4zK #ResearchAtPSI # #Astrophysics #Cerium140 #SpaceResearch #CERN

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