EPJ Web of Conferences
Volume 91, 2015Heavy Ion Accelerator Symposium 2014
|Number of page(s)||4|
|Published online||06 April 2015|
Breakup following interactions with light targets: Investigating new methods to probe nuclear physics input to the cosmological lithium problem.
1 Department of Nuclear Physics, Research School of Physics and Engineering, The Australian National University, Canberra, ACT 0200, Australia
2 Nuclear Physics Division, Bhabha Atomic Research Centre, Trombay, Mumbai - 400085, India
a e-mail: firstname.lastname@example.org
Published online: 6 April 2015
A well known issue with concordance cosmology is the cosmological lithium problem, where models of Big Bang Nucleosynthesis indicate abundances of 7Li three to four times larger than values inferred via spectroscopic measurements of metal-poor halo stars . Since the source of this discrepancy remains unclear , it is vital to fully understand the nuclear reactions that affect the production of 7Li during the Big Bang . At the Australian National University, experimental equipment and analysis techniques have been developed for nuclear reaction studies at energies near the fusion barrier, exploiting large solid angle detectors to enable the investigation of breakup without a priori assumption of the breakup kinematics. The extension to reactions of astrophysical interest may help shed light on these reactions. Recent experiments, using these new techniques, have provided a complete picture of the breakup mechanisms of light nuclei in collisions with heavy targets . The present work focuses on obtaining a complete picture of breakup mechanisms of 7Li following interactions with 27Al. It has been found that breakup is almost exclusively triggered by nucleon transfer between the colliding partners, to a larger extent than was found for heavier targets. The findings of these experiments, as well as progress towards extensions to astrophysically relevant reactions, such as d + 7Be  will be presented.
© Owned by the authors, published by EDP Sciences, 2015
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