Description
Abstract:After a brief introduction to the present state of art of nuclear beta-decay studies in astrophysics, we report our recent work on the long-standing ⁹⁹Tc problem. Having combined a detailed study of the recurrent He-shell thermal-pulse, third dredge-up episodes in a 2.25 M/sub solar/ star and an s-process network calculation, we show that a substantial amount of ⁹⁹Tc can be produced by the s-process and can survive to be dredged up to the stellar surface. We stress that the factual observation of ⁹⁹Tc at the surface of certain stars does not necessarily preclude the ²²Ne(..cap alpha..,n)²⁵Mg reaction from remaining as the neutron source for the s-process. The calculated surface abundances of ⁹⁹Tc and elements with neighboring atomic numbers are compared with observations. 43 refs., 5 figs.
Item Description:Published through the Information Bridge: DOE Scientific and Technical Information.
05/30/1985.
"ucrl-92789"
" conf-850375-12"
"DE85014182"
20. Recontre de Moriond, Les Arcs, France, 10 Mar 1985.
Becker, S.A.; Mathews, G.J.; Ward, R.A.; Takahashi, K.
Physical Description:Pages: 10 : digital, PDF file.