Using Inertial Fusion Implosions to Measure the T + [superscript 3]He Fusion Cross Section at Nucleosynthesis-Relevant Energies
Light nuclei were created during big-bang nucleosynthesis (BBN). Standard BBN theory, using rates inferred from accelerator-beam data, cannot explain high levels of [superscript 6]Li in low-metallicity stars. Using high-energy-density plasmas we measure the T([superscript 3]He,γ)[superscript 6]Li re...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , |
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Other Authors: | |
Format: | Article |
Language: | English |
Published: |
American Physical Society
2017
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Online Access: | http://hdl.handle.net/1721.1/109553 https://orcid.org/0000-0003-0489-7479 https://orcid.org/0000-0002-6919-4881 https://orcid.org/0000-0001-7274-236X https://orcid.org/0000-0002-1020-3501 |