The 3He (α, γ) 7Be S-factor at solar energies: The prompt γ experiment at LUNA

Nuclear Physics A

Volumn 814, Issue 1-4, 2008, Pages 144-158

  Costantini, H ^a   Bemmerer, D ^b   Confortola, F ^a   Formicola, A ^c   Gyurky Gy ^d   Bezzon, P ^e   Bonetti, R ^f   Broggini, C ^e   Corvisiero, P ^a   Elekes, Z ^d   Fulop Zs ^d   Gervino, G ^g   Guglielmetti, A ^f   Gustavino, C ^c   Imbriani, G ^h   Junker, M ^c   Laubenstein, M ^c   Lemut, A ^a   Limata, B ^h   Lozza, V ^e   Marta, M ^f   Menegazzo, R ^e   Prati, P ^a   Roca, V ^h   Rolfs, C ⁱ   Alvarez, C Rossi ^e   Somorjai, E ^d   Straniero, O ^j   Strieder, F ⁱ   Terrasi, F ^k   Trautvetter, H P ⁱ   more..

^a UNIVERSITY OF GENOA   (Italy)

^b INSTITUTE OF ION BEAM PHYSICS AND MATERIALS RESEARCH   (Germany)

^c LABORATORI NAZIONALI DEL GRAN SASSO   (Italy)

^d INSTITUTE OF NUCLEAR RESEARCH ATOMKI   (Hungary)

^e SEZIONE DI PADOVA   (Italy)

^f UNIVERSITY OF MILAN   (Italy)

^g UNIVERSITY OF TURIN   (Italy)

^h UNIVERSITY OF NAPLES FEDERICO II   (Italy)

ⁱ RUHR UNIVERSITY BOCHUM   (Germany)

^j INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^k SECOND UNIVERSITY OF NAPLES   (Italy)

more..

Author keywords

; 3He ( , ) 7Be; astrophysical S factor; branching ratio; Comparison with other data; deduced; E = 220, 250, 400 keV; E ; HPGe detector in the Gran Sasso undreground laboratory; I ; measured; Nuclear reactions; Prompt texhnique

Indexed keywords

EID: 56249108047     PISSN: 03759474     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.nuclphysa.2008.09.014     Document Type: Article

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