ISF 3.6

Comparison of the Gamow-Teller strength distribution in 58Co extracted from
58Ni(t,3He) data at 115 MeV/nucleon [Col06] and large-scale shell model calculations [Hag04],
with the GXPF1 interaction [Hon04] (top left) and the KB3G interaction [Pov01] (top right). The
bottom panel shows electron-capture rates based on the experimental and theoretical Gamow-
Teller strength distributions and for conditions during the precollapse stage of a massive star
(density (ρ) times electron fraction (Ye) of 107 gcm-3). Adapted from [Col06].

References:
[Col06] A.L. Cole et al., Phys. Rev. C 74, 034333 (2006)
[Hag04] M. Hagemann et al., Phys. Lett. B 579, 251 (2004)
[Hon04] M. Honma et al., Phys. Rev. C 69, 034335 (2004)
[Pov01] A. Poves et al., Nucl. Phys. A 694, 157 (2001)
[Col06] A.L. Cole et al., Phys. Rev. C 74, 034333 (2006)