
The Trojan horse method in nuclear astrophysics: recent results
2007; IOP Publishing; Volume: 35; Issue: 1 Linguagem: Inglês
10.1088/0954-3899/35/1/014008
ISSN1361-6471
AutoresS. Romano, C. Spitaleri, S. Cherubini, V. Crucillà, M. Gulino, M. La Cognata, L. Lamia, R. G. Pizzone, Chengbo Li, G. G. Rapisarda, M. L. Sergi, S. Tudisco, А. Туміно, R. E. Tribble, V. Z. Goldberg, A. M. Mukhamedzhanov, G. Tăbăcaru, L. Trache, V. Kroha, V. Burjan, Z. Hons, J. Mrázek, E. Somorjai, Z. Elekes, Zsolt Fülöp, Gy. Gyürky, G. Kiss, A. Szanto de Toledo, N. Carlin, M. M. de Moura, M. G. Del Santo, M. G. Munhoz, R. Liguori Neto, F. A. Souza, A. A. P. Suaide, E. M. Szanto,
Tópico(s)Nuclear Physics and Applications
ResumoDifficulties in cross-section measurements at very low energies, when charged particles are involved, led to the development of some indirect methods. The Trojan horse method (THM) allows us to bypass the Coulomb effects and has been successfully applied to several reactions of astrophysical interest. A brief review of the THM applications is reported together with some of the most recent results.
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