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Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV
The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have perf...
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Published in: | Physical review letters 2024-02, Vol.132 (6), p.062702 |
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container_title | Physical review letters |
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creator | deBoer, R J Febbraro, M Bardayan, D W Boomershine, C Brandenburg, K Brune, C Coil, S Couder, M Derkin, J Dede, S Fang, R Fritsch, A Gula, A Gyürky, Gy Hackett, B Hamad, G Jones-Alberty, Y Kelmar, R Manukyan, K Matney, M McDonaugh, J Meisel, Z Moylan, S Nattress, J Odell, D O'Malley, P Paris, M W Robertson, D Shahina Singh, N Smith, K Smith, M S Stech, E Tan, W Wiescher, M |
description | The cross section of the ^{13}C(α,n)^{16}O reaction is needed for nuclear astrophysics and applications to a precision of 10% or better, yet inconsistencies among 50 years of experimental studies currently lead to an uncertainty of ≈15%. Using a state-of-the-art neutron detection array, we have performed a high resolution differential cross section study covering a broad energy range. These measurements result in a dramatic improvement in the extrapolation of the cross section to stellar energies potentially reducing the uncertainty to ≈5% and resolving long standing discrepancies in higher energy data. |
doi_str_mv | 10.1103/PhysRevLett.132.062702 |
format | article |
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title | Measurement of the ^{13}C(α, n_{0})^{16}O Differential Cross Section from 0.8 to 6.5 MeV |
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