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Nuclear Physics Mid Term Plan at LNGS

https://doi.org/10.1140/epjp/s13360-023-04840-2

Buompane, R; Cavanna, F; Curceanu, C; D’Onofrio, A; Di_Leva, A; Formicola, A; Gialanella, L; Gustavino, C; Imbriani, G; Junker, M; et al (March 2024, The European Physical Journal Plus)

Abstract The Istituto Nazionale di Fisica Nucleare—Laboratori Nazionali del Gran Sasso (LNGS) is one of the largest underground physics laboratory, a very peculiar environment suited for experiments in Astroparticle Physics, Nuclear Physics and Fundamental Symmetries. The newly established Bellotti Ion Beam facility represents a major advance in the possibilities of studying nuclear processes in an underground environment. A workshop was organized at LNGS in the framework of the Nuclear Physics Mid Term Plan in Italy, an initiative of the Nuclear Physics Division of the Instituto Nazionale di Fisica Nucleare to discuss the opportunities that will be possible to study in the near future by employing state-of-the-art detection systems. In this report, a detailed discussion of the outcome of the workshop is presented.
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Experimental studies on astrophysical reactions at the low-energy RI beam separator CRIB

https://doi.org/10.1051/epjconf/202226003003

Yamaguchi, H.; Hayakawa, S.; Ma, N.R.; Shimizu, H.; Okawa, K.; Yang, L.; Kahl, D.; La Cognata, M.; Lamia, L.; Abe, K.; et al (January 2022, EPJ Web of Conferences)
Liu, W.; Wang, Y.; Guo, B.; Tang, X.; Zeng, S. (Ed.)
Experimental studies on astrophysical reactions involving radioactive isotopes (RI) often accompany technical challenges. Studies on such nuclear reactions have been conducted at the low-energy RI beam separator CRIB, operated by Center for Nuclear Study, the University of Tokyo. We discuss two cases of astrophysical reaction studies at CRIB; one is for the 7 Be+ n reactions which may affect the primordial 7 Li abundance in the Big-Bang nucleosynthesis, and the other is for the 22 Mg( α , p ) reaction relevantin X-raybursts.
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Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New ${}^{22}{Mg} (α, p) {}^{25}{Al}$ Reaction Rate Determined at the Gamow Energy

https://doi.org/10.1103/PhysRevLett.127.172701

Hu, J.; Yamaguchi, H.; Lam, Y. H.; Heger, A.; Kahl, D.; Jacobs, A. M.; Johnston, Z.; Xu, S. W.; Zhang, N. T.; Ma, S. B.; et al (October 2021, Physical Review Letters)
Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient (ANC) method

https://doi.org/10.1016/j.physletb.2020.135606

Kiss, G.G.; La Cognata, M.; Spitaleri, C.; Yarmukhamedov, R.; Wiedenhöver, I.; Baby, L.T.; Cherubini, S.; Cvetinović, A.; D'Agata, G.; Figuera, P.; et al (August 2020, Physics Letters B)
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