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Creators/Authors contains: "Romano, S"

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  1. ; ; ; ; ; ; ; ; ; ; et al (, Physical Review Letters)
  2. ; ; ; ; ; ; ; ; ; ; et al (, The Astrophysical Journal)
    Abstract Neutron-induced nuclear reactions play an important role in the Big Bang Nucleosynthesis. Their excitation functions are, from an experimental point of view, usually difficult to measure. Nevertheless, in the last decades, big efforts have led to a better understanding of their role in the primordial nucleosynthesis network. In this work, we apply the Trojan Horse Method to extract the cross section at astrophysical energies for the3He(n,p)3H reaction after a detailed study of the2H(3He,pt)H three-body process. Data extracted from the present measurement are compared with other published sets. The reaction rate is also calculated, and the impact on the Big Bang nucleosynthesis is examined in detail. 
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    Free, publicly-accessible full text available November 1, 2025
  3. ; ; ; ; ; ; ; ; ; ; et al (, 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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  4. ; ; ; ; ; ; ; ; ; ; et al (, EPJ Web of Conferences)
    In the network of reactions present in the Big Bang nucleosynthesis, the 3 He(n, p) 3 H has an important role which impacts the final 7 Li abundance. The Trojan Horse Method (THM) has been applied to the 3 He(d, pt)H reaction in order to extract the astrophysical S(E)-factor of the 3 He(n, p ) 3 H in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results. 
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  5. ; ; ; ; ; ; ; ; ; ; et al (, 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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  6. ; ; ; ; ; ; ; ; ; ; et al (, Physical Review Letters)
  7. ; ; ; ; ; ; ; ; ; ; et al (, Journal of Physics: Conference Series)
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  8. ; ; ; ; ; ; ; ; ; ; et al (, Physics Letters B)
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  9. ; ; ; ; ; ; ; ; ; ; et al (, The European Physical Journal A)
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