Origin of 48Ca

Physics – Nuclear Physics

Scientific paper

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Scientific paper

We stress conceptual understanding of why 48Ca survives low-entropy expansions but not high-entropy expansions. Type Ia supernovae are thereby demonstrated to be its source. The interdependence of the quasiequilibrium cluster (QSE) and the number of heavy nuclei is the key. By varying reaction rates, we show that nuclear cross sections are not a sensitive need for the problem of 48Ca nucleosynthesis.

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