M E Bennett et al 2010 J. Phys.: Conf. Ser. 202 012023 doi:10.1088/1742-6596/202/1/012023
M E Bennett1, R Hirschi1,2, M Pignatari7,3,4, S Diehl5, C Fryer6, F Herwig7, A Hungerford6, G Magkotsios3,8, G Rockefeller6, F Timmes8, M Wiescher3 and P Young8
Show affiliationsThe slow neutron capture process in massive stars (the weak s-process) produces most of the s-only isotopes in the mass region 60 < A < 90. The nuclear reaction rates used in simulations of this process have a profound effect on the final s-process yields. We generated 1D stellar models of a 25M
star varying the 12C + 12C rate by a factor of 10 and calculated full nucleosynthesis using the post-processing code PPN. Increasing or decreasing the rate by a factor of 10 affects the convective history and nucleosynthesis, and consequently the final yields.
27.30.+t 20(less-than-or-equal-to)A(less-than-or-equal-to)38
27.20.+n 6(less-than-or-equal-to)A(less-than-or-equal-to)19
97.10.Cv Stellar structure, interiors, evolution, nucleosynthesis, ages
Issue 1 (2010)
M E Bennett et al 2010 J. Phys.: Conf. Ser. 202 012023
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