Measuring the Radiative Width of the Hoyle State in $^{12}$C
ORAL
Abstract
In stellar nucleosynthesis the conversion of helium into heavier elements begins with the triple-$\alpha$ process, in which three $\alpha$ particles combine to form $^{12}$C. The rate of this process is governed by the 0$^+$ second excited state of $^{12}$C which provides a resonance for the $\alpha$+$^{8}$Be$\rightarrow$ $^{12}$C* at an excitation energy 7.65 MeV (the Hoyle state). Overwhelmingly, the 7.65 MeV state decays by $\alpha$ particle to $^8$Be which then breaks up into two $\alpha$ particles. However, there is a small radiative decay branch (approximately 4$\times10^{-4}$) which allows the excited $^{12}$C* nucleus to decay to its ground state. A new measurement of the ratio of the radiative width to the total width has been performed by the Lawrence Livermore National Laboratory and Lawrence Berkeley National Laboratory STARS/LIBERACE collaboration. Current results and the our experimental method will be presented.
*This work was sponsored by UC-LLNL under Contract No. W-7405-Eng-48 and Grant Nos. DE-FG-05NA25929, DE-FG52-06NA26206, and DE-FG02-05ER41379.
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