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0544735 - ÚJF 2022 RIV US eng J - Journal Article
Kiss, G. G. - La Cognata, M. - Yarmukhamedov, R. - Tursunmakhatov, K. I. - Wiedenhover, I. - Baby, L. T. - Cherubini, S. - Cvetinovic, A. - D'Agata, Giuseppe - Figuera, P. - Guardo, G. L. - Gulino, M. - Hayakawa, S. - Indelicato, I. - Lamia, L. - Lattuada, M. - Mudo, F. - Palmerini, S. - Pizzone, R. G. - Rapisarda, G. G. - Romano, S. - Sergi, M. L. - Sparta, R. - Spitaleri, C. - Trippella, O. - Tumino, A. - Anastasiou, M. - Kuvin, S. A. - Rijal, N. - Schmidt, B. - Igamov, S. B. - Sakuta, S. B. - Fulop, Z. - Gyurky, G. - Szucs, T. - Halasz, Z. - Somorjai, E. - Hons, Zdeněk - Mrázek, Jaromír - Tribble, R. E. - Mukhamedzhanov, A. M.
Indirect determination of the astrophysical S factor for the Li-6(p, gamma) Be-7 reaction using the asymptotic normalization coefficient method.
Physical Review C. Roč. 104, č. 1 (2021), č. článku 015807. ISSN 2469-9985. E-ISSN 2469-9993
R&D Projects: GA MŠMT(CZ) EF16_013/0001679
Institutional support: RVO:61389005
Keywords : astrophysical S factor * ANC method * nuclear reaction
OECD category: Astronomy (including astrophysics,space science)
Impact factor: 3.199, year: 2021
Method of publishing: Limited access
https://doi.org/10.1103/PhysRevC.104.015807
Permanent Link: http://hdl.handle.net/11104/0321557