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NSR database version of May 6, 2024.

Search: Author = B.Soos

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2022LU09      Universe 8, 343 (2022)

M.Lugaro, A.Yague Lopez, B.Soos, B.Cote, M.Peto, N.Vassh, B.Wehmeyer, M.Pignatari

Origin of Plutonium-244 in the Early Solar System

ATOMIC MASSES ^127,129In, ^235,238U, ²⁴⁴Pu, ²⁴⁷Cm; calculated ratios of abundances of ¹²⁹I/¹²⁷I, ¹²⁹I/²⁴⁷Cm, ²⁴⁴Pu/²³⁸U, and ²⁴⁷Cm/²³⁵U produced as short-lived radionucldies (SLRs) in r-process, and present in the early Solar System (ESS) using nuclear network code WINNET with 63 different models, and the nucleosynthesis network PRISM with 14 different models, with detailed results listed in the Supplementary Materials of the paper. ²⁴⁴Pu; discussed different possibilities, solutions, and derived time intervals for the presence of this isotope in early Solar System.

doi: 10.3390/universe8070343
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