| Autor: |
D. Blankstein, Lauren Callahan, G. G. Rapisarda, C. Seyymour, Livio Lamia, G. L. Guardo, C. Spampinato, D. Bardyan, M. L. Sergi, L. Boccioli, Manoel Couder, Roberta Spartà, P. M. Prajapati, A. M. Clark, V. Burian, Austin Nelson, Sean R. McGuinness, G. D’Agata, A. Tumino, M. La Cognata, Michael Skulski, K. Y. Chae, J. Long, Q. Liu, Ashabari Majumdar, Rebeka Kelmar, C. Spitaleri, John Wilkinson, S. Romano, A. A. Oliva, Patrick O'Malley, S. L. Henderson, J. Mrazek, R. G. Pizzone, I. Indelicato, D. Lattuada, Michael Wiescher, M. R. Hall, A. Gula, B. Frentz, S. Anguilar, W. Tan, Sara Palmerini |
| Jazyk: |
angličtina |
| Rok vydání: |
2020 |
| Předmět: |
|
| Zdroj: |
EPJ Web of Conferences, Vol 227, p 02013 (2020) |
| Popis: |
In the network of reactions present in the Big Bang nucleosynthesis, the 3He(n, p)3H has an important role which impacts the final 7Li abundance. The Trojan Horse Method (THM) has been applied to the 3He(d, pt)H reaction in order to extract the astrophysical S(E)-factor of the 3He(n, p)3H in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results. |
| Databáze: |
OpenAIRE |
| Externí odkaz: |
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