Abstract
The disagreement between observed 7Li abundances in metal-poor halo stars and primordial 7Li abundances predicted in Big Bang Nucleosynthesis (BBN) calculations has presented a challenge to the astrophysics community for some time. The absence of a clear astrophysical explanation of this problem has reignited a search for a possible nuclear solution. The Nuclear Reaction Dynamics group at the Australian National University has recently developed the Break-up Array for LIght Nuclei (BALIN), a new highly pixelated detector array capable of providing the most complete picture of nuclear reactions leading to the breakup of light nuclei. First measurements with this array have already yielded surprising new information about the breakup dynamics of sub-barrier collisions between 6,7Li and 208Pb. Results from these measurements are presented as a demonstration of the array's capabilities. Possible implications for reactions of relevance to BBN will be explored in the future.
Original language | English |
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Journal | Proceedings of Science |
Publication status | Published - 2012 |
Event | 12th International Symposium on Nuclei in the Cosmos, NIC 2012 - Cairns, QLD, Australia Duration: 5 Aug 2012 → 12 Aug 2012 |