Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..78...85c&link_type=abstract
Astrophysics and Space Science, Volume 78, Issue 1, pp.85-94
Astronomy and Astrophysics
Astrophysics
46
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.
Cosner Kenneth
Truran James W.
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