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Abstract
The accurate knowledge of thermonuclear reaction rates is important in understanding the energy generation, the neutrinos luminosity and the synthesis of elements in stars. The physical conditions under which the majority of astrophysical reactions proceed in stellar environments make it difficult or impossible to measure them under the same conditions in the laboratory. That is why different indirect techniques are being used along with direct measurements. The Trojan Horse Method (THM) is introduced as an independent technique to obtain the bare nucleus astrophysical S(E)-factor. As examples the results of recent the application of THM to the 2H(11B, σ08Be)n and 2H(10B, σ07Be)n reactions are presented.
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1 Dipartimento di Fisica e Astronomia, Università di Catania, Catania, Italy; INFN, Laboratori Nazionali del Sud, Catania, Italy
2 Departamento de Física Nuclear, Universitade de Sao Paulo, Sao Paulo, Brasil
3 Nuclear Physics Institute of ASCR, Rez, Czech Republic
4 Beijing Radiation Center, 100875 Beijing, China
5 INFN, Laboratori Nazionali del Sud, Catania, Italy
6 GIK Institute of Engineering Sciences and Technology, Topi, Districti Swabi, K.P. Pakistan
7 Cyclotron Institute, Texas A&M University, College Station, TX 77843, USA
8 China Institute of Atomic Energy, Beijing, China
9 Institute for Nuclear Research (ATOMKI), Debrecen, Hungary
10 INFN, Laboratori Nazionali del Sud, Catania, Italy; University of Enna, Unikore, Enna, Italy
11 China
12 CNS-University of Tokio, Japan