A new setup for the underground study of capture reactions
- C. Casella
- H. Costantini
- A. Lemut
- B. Limata
- D. Bemmerer
- R. Bonetti
- C. Broggini
- L. Campajola
- P. Cocconi
- P. Corvisiero
- J. Cruz
- A. D’Onofrio
- A. Formicola
- Z. Fülöp
- G. Gervino
- L. Gialanella
- A. Guglielmetti
- C. Gustavino
- G. Gyurky
- A. Loiano
- A. P. Jesus
- M. Junker
- P. Musico
- A. Ordine
- F. Parodi
- M. Parolin
- J. V. Pinto
- P. Prati
- J. P. Ribeiro
- D. Rogalla
- C. Rolfs
- C. Rossi Alvarez
- A. Rottura
- F. Schuemann
- E. Somorjai
- F. Strieder
- F. Terrasi
- H. P. Trautvetter
- A. Vomiero
- S. Zavatarelli
- IMBRIANI, GIANLUCA
- ROCA, VINCENZO
- ROMANO, MARIO
Publication date
January 2002
DOIAbstract
For the study of astrophysically relevant capture reactions in the underground laboratory LUNA a new setup of high sensitivity has been implemented. The setup includes a windowless gas target, a 4pi BGO summing crystal, and beam calorimeters. The setup has been recently used to measure the d(p,gamma)He-3 cross-section for the first time within its solar Gamow peak, i.e. down to 2.5 keV c.m. energy. The features of the optimized setup are described
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