TY - JOUR
T1 - Direct capture cross sections at low energy
AU - Williams, R. D.
AU - Koonin, S. E.
N1 - Funding Information:
Dr Lokhandwala and Ms Farrelly are employees of Xcenda LLC; Xcenda received funding from GSK to support the conduct of this study and did not receive funding for manuscript development. Mr Acharya and Dr Coutinho were employees of Xcenda LLC during the conduct of the study. Mr Bell and Dr Svedsater are employees of, and hold stocks/shares in, GSK. This study was funded by GSK (study 216974) and Vir Biotechnology, Inc. The study sponsors were involved in the study design; collection, analysis, and interpretation of data; writing of the report; and the decision to submit the report for publication.
Funding Information:
The authors would like to acknowledge Helen Birch (GSK) for her contribution to the study design, interpretation of results, and critical review of the manuscript. Editorial support (in the form of writing assistance, including preparation of the draft manuscript under the direction and guidance of the authors, collating and incorporating authors’ comments for each draft, assembling tables and figures, grammatical editing, and referencing) was provided by Kathryn Wardle and Tony Reardon of Aura, a division of Spirit Medical Communications Group Limited (Manchester, UK), and was funded by GSK. All data relevant to the study are included in the article or uploaded as supplementary information. All data required for interpretation of these results are included in this manuscript.
PY - 1981
Y1 - 1981
N2 - We derive simple expressions for the low-energy behavior of direct radiative capture cross sections, particularly those important in solar nucleosynthesis, such as He3()Be7, H3()Li7, and Be7(p,)B8. Our results for the He3()Be7 reaction are inconsistent with a measurement by Rolfs et al. NUCLEAR REACTIONS He3()Be7, H3()Li7, E<300 keV, Be7(p,)B8, E<100 keV, extrapolated S.
AB - We derive simple expressions for the low-energy behavior of direct radiative capture cross sections, particularly those important in solar nucleosynthesis, such as He3()Be7, H3()Li7, and Be7(p,)B8. Our results for the He3()Be7 reaction are inconsistent with a measurement by Rolfs et al. NUCLEAR REACTIONS He3()Be7, H3()Li7, E<300 keV, Be7(p,)B8, E<100 keV, extrapolated S.
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U2 - 10.1103/PhysRevC.23.2773
DO - 10.1103/PhysRevC.23.2773
M3 - Article
AN - SCOPUS:4244092931
SN - 0556-2813
VL - 23
SP - 2773
EP - 2774
JO - Physical Review C
JF - Physical Review C
IS - 6
ER -