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.

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; Imbriani, Gianluca; A. P., Jesus; M., Junker; P., Musico; A., Ordine; F., Parodi; M., Parolin; J. V., Pinto; P., Prati; J. P., Ribeiro; Roca, Vincenzo; D., Rogalla; C., Rolfs; Romano, Mario; C., Rossi Alvarez; A., Rottura; F., Schuemann; E., Somorjai; F., Strieder; F., Terrasi; H. P., Trautvetter; A., Vomiero; S., Zavatarelli. - In: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT. - ISSN 0168-9002. - STAMPA. - 489:1-3(2002), pp. 160-169. [10.1016/S0168-9002(02)00577-6]

A new setup for the underground study of capture reactions

IMBRIANI, GIANLUCA;ROCA, VINCENZO;ROMANO, MARIO;
2002

Abstract

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.
2002
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; Imbriani, Gianluca; A. P., Jesus; M., Junker; P., Musico; A., Ordine; F., Parodi; M., Parolin; J. V., Pinto; P., Prati; J. P., Ribeiro; Roca, Vincenzo; D., Rogalla; C., Rolfs; Romano, Mario; C., Rossi Alvarez; A., Rottura; F., Schuemann; E., Somorjai; F., Strieder; F., Terrasi; H. P., Trautvetter; A., Vomiero; S., Zavatarelli. - In: NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH. SECTION A, ACCELERATORS, SPECTROMETERS, DETECTORS AND ASSOCIATED EQUIPMENT. - ISSN 0168-9002. - STAMPA. - 489:1-3(2002), pp. 160-169. [10.1016/S0168-9002(02)00577-6]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/510517
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