Trojan Horse Method: recent results in nuclear astrophysics
Autor: | Silvio Cherubini, Qungang Wen, J. Mrazek, Livio Lamia, H. Yamaguchi, M. Mukhamedzhanov, L. Sergi, V. Kroha, N. Carlin, Marcelo Gameiro Munhoz, C. Spitaleri, M. R. Puglia, B. F. Irgaziev, S. Romano, Sara Palmerini, G. Tabacaru, R. G. Pizzone, M. Gimenez del Santo, A. Tumino, Yusuke Wakabayashi, Marisa Gulino, V. Burjan, G. G. Rapisarda, Chengbo Li, A. Szanto de Toledo, M. La Cognata, E. Somorjai, Z. Hons, S. Zhou, F. A. Souza, V. Crucillà |
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Jazyk: | angličtina |
Rok vydání: | 2015 |
Předmět: |
Physics
History RELEVANT Thermonuclear reaction Trojan horse Astrophysics Measure (mathematics) Computer Science Applications Education Luminosity Nuclear physics Stars Physics and Astronomy (all) LOW-ENERGY BORON DEPLETION REACTION-RATES CROSS-SECTION RELEVANT Nuclear astrophysics REACTION-RATES BORON DEPLETION LOW-ENERGY Neutrino CROSS-SECTION |
Popis: | 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, ?08Be)n and 2H(10B, ?07Be)n reactions are presented. |
Databáze: | OpenAIRE |
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