Beta Decay Rates for S-Process Studies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The rates for a variety of beta decay processes have been determined as a function of temperature for nuclei which can participate in thes-process production of heavy elements, occurring in the presence of the22Ne(α,n)25 Mg neutron source operating in the convective helium shells of thermally pulsing stars. Specifically: calculated half-lives are presented for electron emission, positron emission, and electron capture over the temperature range 108 109 K.

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