Few-body decay and recombination in nuclear astrophysics

Three-body continuum problems are investigated for light nuclei of astrophysical relevance. We focus on three-body decays of resonances or recombination via resonances or the continuum background. The concepts of widths, decay mechanisms and dynamic evolution are discussed. We also discuss results for the triple $α$ decay in connection with $2^+$ resonances and density and temperature dependence rates of recombination into light nuclei from $α$-particles and neutrons.

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