Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2010-12-28
Physical Review C 81, 052801(R) (2010)
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Published in Phys. Rev. C, 13 pages, 4 figures
Scientific paper
10.1103/PhysRevC.81.052801
We have made a new time-dependent calculation of the supernova production ratio of the long-lived isomeric state of $^{180}$Ta. Such a time-dependent solution is crucial for understanding the production and survival of this isotope. We include the explicit linking between the isomer and all known excited states.We have also calculated the properties of possible links to a conjectured excited state that might decrease the final isomer residual ratio. We find that the explicit time evolution of the synthesis of $^{180}$Ta using the available nuclear data avoids the overproduction relative to $^{138}$La for a $\nu$-process neutrino temperature of 4 MeV.
Chiba Satoshi
Hayakawa Tadaaki
Kajino Taka
Mathews Grant J.
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