Original title: Indirect Approach To The H-2(d,p)H-3 Reaction Study
Authors: Sparta, R. ; Pizzone, R. G. ; Spitaleri, C. ; Aliotta, M. ; Burjan, Václav ; Cherubini, S. ; Crucilla, V. ; Gulino, M. ; Hons, Zdeněk ; Kiss, G. G. ; Kroha, Václav ; La Cognata, M. ; Lamia, L. ; McCleskey, M. ; Mrázek, Jaromír ; Puglia, S. M. R. ; Rapisarda, G. G. ; Romano, S. ; Sergi, M. L. ; Trache, L. ; Tumino, A.
Document type: Papers
Conference/Event: Carphathian Summer School of Physics Conference, Sinaia (RO), 20100620
Year: 2010
Language: eng
Abstract: In order to understand primordial and stellar nucleosynthesis, we have studied H-2(d,p)H-3 reaction at 0.4 MeV down to astrophysical energies. Knowledge of its S-factor is interesting also to plan reactions for fusion reactors to produce energy. The H-2(d,p)H-3 reaction has been studied through the Trojan Horse Method applied to the three-body reaction H-2(He-3,pt)H, at beam energy of 17 MeV. Once selection of protons and tritons detected in coincidence and the selection of quasi-free events, the obtained S-factor is compared with direct measurements. Such data are in agreement with the direct ones and a pole invariance test has been obtained comparing the present results with another H-2(d,p)H-3 THM measurements, where a different spectator particle was employed.
Keywords: Big Bang nucleosynthesis; nuclear astrohphysics; Trojan Horse
Host item entry: AIP Conference Proceedings, ISBN 978-0-7354-0859-3, ISSN 0094-243X

Institution: Nuclear Physics Institute AS ČR (web)
Document availability information: Fulltext is available at the institute of the Academy of Sciences.
Original record: http://hdl.handle.net/11104/0281531

Permalink: http://www.nusl.cz/ntk/nusl-373396


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Research > Institutes ASCR > Nuclear Physics Institute
Conference materials > Papers
 Record created 2018-03-09, last modified 2021-11-24


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