EPJ Web of Conferences (Jan 2020)
Study of 3He(n,p)3H reaction at cosmological energies with trojan horse method
- Spampinato C.,
- Pizzone R.G.,
- Spartà R.,
- Couder M.,
- Tan W.,
- Burian V.,
- Chae K.Y.,
- D’Agata G.,
- Guardo G.L.,
- Indelicato I.,
- Cognata M. La,
- Lamia L.,
- Lattuada D.,
- Mrazek J.,
- Oliva A.,
- Palmerini S.,
- Prajapati P.M.,
- Rapisarda G.G.,
- Romano S.,
- Sergi M.L.,
- Spitaleri C.,
- Tumino A.,
- Wiescher M.,
- Anguilar S.,
- Bardyan D.,
- Blankstein D.,
- Boccioli L.,
- Callahan L.,
- Clark A.,
- Frentz B.,
- Hall M.,
- Gula A.,
- Henderson S.,
- Kelmar R.,
- Liu Q.,
- Long J.,
- Majumdar A.,
- McGuinness S.,
- Nelson A.,
- O’Malley P.,
- Seyymour C.,
- Skulski M.,
- Wilkinson J.
Affiliations
- Spampinato C.
- Pizzone R.G.
- Laboratori Nazionali del Sud, INFN
- Spartà R.
- Couder M.
- Physics and Astronomy Department, Notre Dame University
- Tan W.
- Centro Siciliano di Fisica Nucleare e Struttura della Materia
- Burian V.
- Cyclotron Institute, Academy of Science of the Czech Rep.
- Chae K.Y.
- SKKU Sungkyunkwan University
- D’Agata G.
- Cyclotron Institute, Academy of Science of the Czech Rep.
- Guardo G.L.
- Laboratori Nazionali del Sud, INFN
- Indelicato I.
- Laboratori Nazionali del Sud, INFN
- Cognata M. La
- Laboratori Nazionali del Sud, INFN
- Lamia L.
- Lattuada D.
- Kore University
- Mrazek J.
- Cyclotron Institute, Academy of Science of the Czech Rep.
- Oliva A.
- Laboratori Nazionali del Sud, INFN
- Palmerini S.
- INFN and University of Perugia
- Prajapati P.M.
- Laboratori Nazionali del Sud, INFN
- Rapisarda G.G.
- Laboratori Nazionali del Sud, INFN
- Romano S.
- Sergi M.L.
- Laboratori Nazionali del Sud, INFN
- Spitaleri C.
- Tumino A.
- Wiescher M.
- Physics and Astronomy Department, Notre Dame University
- Anguilar S.
- Physics and Astronomy Department, Notre Dame University
- Bardyan D.
- Physics and Astronomy Department, Notre Dame University
- Blankstein D.
- Physics and Astronomy Department, Notre Dame University
- Boccioli L.
- Callahan L.
- Physics and Astronomy Department, Notre Dame University
- Clark A.
- Physics and Astronomy Department, Notre Dame University
- Frentz B.
- Physics and Astronomy Department, Notre Dame University
- Hall M.
- Physics and Astronomy Department, Notre Dame University
- Gula A.
- Physics and Astronomy Department, Notre Dame University
- Henderson S.
- Physics and Astronomy Department, Notre Dame University
- Kelmar R.
- Physics and Astronomy Department, Notre Dame University
- Liu Q.
- Physics and Astronomy Department, Notre Dame University
- Long J.
- Physics and Astronomy Department, Notre Dame University
- Majumdar A.
- Physics and Astronomy Department, Notre Dame University
- McGuinness S.
- Physics and Astronomy Department, Notre Dame University
- Nelson A.
- Physics and Astronomy Department, Notre Dame University
- O’Malley P.
- Physics and Astronomy Department, Notre Dame University
- Seyymour C.
- Physics and Astronomy Department, Notre Dame University
- Skulski M.
- Physics and Astronomy Department, Notre Dame University
- Wilkinson J.
- Physics and Astronomy Department, Notre Dame University
- DOI
- https://doi.org/10.1051/epjconf/202022702013
- Journal volume & issue
-
Vol. 227
p. 02013
Abstract
In the network of reactions present in the Big Bang nucleosynthesis, the 3He(n, p)3H has an important role which impacts the final 7Li abundance. The Trojan Horse Method (THM) has been applied to the 3He(d, pt)H reaction in order to extract the astrophysical S(E)-factor of the 3He(n, p)3H in the Gamow energy range. The experiment will be described in the present work together with the first preliminary results.
