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Enhanced $S$-factor for the $^{14}$N$(p,γ)^{15}$O reaction and its impact on the solar composition problem

Fuente: arXiv

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Bibliographic Details
Main Authors:	Chen, X., Su, J., Shen, Y. P., Zhang, L. Y., He, J. J., Chen, S. Z., Wang, S., Shen, Z. L., Lin, S., Song, L. Y., Zhang, H., Wang, L. H., Jiang, X. Z., Wang, L., Huang, Y. T., Qin, Z. W., Liu, F. C., Sheng, Y. D., Chen, Y. J., Lu, Y. L., Li, X. Y., Dong, J. Y., Jiang, Y. C., Zhang, Y. Q., Zhang, Y., Tian, J. W., Xiao, D., Li, Z. M., Han, X. C., Wei, J. J., Li, H., An, Z., Lin, W. P., Liao, B., Liu, H. N., Zhang, F. S., Qiu, M. L., Xu, C., Jin, S. L., Lu, F., Chen, J. F., Nan, W., Wang, Y. B., Li, Z. H., Guo, B., Gu, Y. Q., Liu, W. P.
Format:	Preprint
Published:	2024
Subjects:	Nuclear Experiment Solar and Stellar Astrophysics
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2410.16086