Using Inertial Fusion Implosions to Measure the T + [superscript 3]He Fusion Cross Section at Nucleosynthesis-Relevant Energies

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...

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Main Authors: Herrmann, H. W., Kim, Y. H., Hale, G., Rubery, M., Paris, M., Bacher, A., Brune, C. R., Forrest, C., Glebov, V. Yu., Janezic, R., McNabb, D., Nikroo, A., Pino, J., Sangster, T. C., Seka, W., Stoeckl, C., Zylstra, Alex Bennett, Gatu Johnson, Maria, Frenje, Johan A, Li, Chikang, Seguin, Fredrick Hampton, Sio, Hong Weng, Petrasso, Richard D
其他作者: Massachusetts Institute of Technology. Department of Physics
格式: 文件
语言:English
出版: American Physical Society 2017
在线阅读: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

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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

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