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NSR database version of May 10, 2024.

Search: Author = K.Spenneberg

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2014HE14      Phys.Rev. C 90, 015802 (2014)

S.Helmrich, K.Spenneberg, A.Palffy

Coupling highly excited nuclei to the atomic shell in dense astrophysical plasmas

NUCLEAR REACTIONS 187Os, 193Ir(n, γ), E=low; calculated σ, stellar mitigation factor (SMF) for an intermediate nuclear excitation by electron capture (NEEC) or photoabsorption (PA) step in stellar plasma environments, reaction rates. Relevance to astrophysical s-process, and 187Re - 187Os cosmochronometer.

doi: 10.1103/PhysRevC.90.015802
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