NSR Query Results

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NSR database version of April 27, 2024.

Search: Author = F.Schuemann

Found 2 matches.

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1999BO23      Phys.Rev.Lett. 82, 5205 (1999)

R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Alessandro, M.Dessalvi, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.Prati, V.Roca, C.Rolfs, M.Romano, F.Schuemann, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli, and the LUNA Collaboration

First Measurement of the ³He(³He, 2p)⁴He Cross Section Down to the Lower Edge of the Solar Gamow Peak

NUCLEAR REACTIONS ³He(³He, 2p), E(cm)=16.5-24.4 keV; measured σ, astrophysical S-factor; deduced electron screening effect, no narrow resonance.

doi: 10.1103/PhysRevLett.82.5205
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0379.

1999PR12      Nucl.Phys. (Supplement) A654, 920c (1999)

P.Prati, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Alessandro, M.Dessalvi, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, M.Junker, A.Ordine, V.Roca, C.Rolfs, M.Romano, F.Schuemann, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli

The LUNA Facility at the National Laboratory of Gran Sasso: Recent results and future activities

NUCLEAR REACTIONS ³He(³He, 2p), E(cm)=16-25 keV; measured astrophysical S-factors, upper limits. Plans for future experiments discussed.

doi: 10.1016/S0375-9474(00)88573-5
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