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First measurement of the d(p,γ)3He cross section down to the solar Gamow peak

✍ Scribed by C. Casella; H. Costantini; A. Lemut; B. Limata; R. Bonetti; C. Broggini; L. Campajola; P. Corvisiero; J. Cruz; A. D'Onofrio; A. Formicola; Z. Fülöp; G. Gervino; L. Gialanella; A. Guglielmetti; C. Gustavino; G. Gyurky; G. Imbriani; A.P. Jesus; M. Junker; A. Ordine; J.V. Pinto; P. Prati; J.P. Ribeiro; V. Roca; D. Rogalla; C. Rolfs; M. Romano; C. Rossi-Alvarez; F. Schuemann; E. Somorjai; O. Straniero; F. Strieder; F. Terrasi; H.P. Trautvetter; S. Zavatarelli

Book ID
104335538
Publisher
Elsevier Science
Year
2002
Tongue
English
Weight
234 KB
Volume
706
Category
Article
ISSN
0375-9474

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✦ Synopsis

Using the 50 kV LUNA accelerator facility at the Gran Sasso underground laboratory we measured, with an accuracy of the order of 10%, the d(p, γ) 3 He cross section from 22 down to

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The cross section of 3He(3He,2p)4He measured at solar energies
✍ M. Junker; C. Arpesella; E. Bellotti; C. Broggini; P. Corvisiero; A. D'Alessandr 📂 Article 📅 1999 🏛 Elsevier Science 🌐 English ⚖ 394 KB

We report on the status of the 3He(3He,2p)4He experiment at the underground accelerator facility LUNA (Gran !&so). The lowest projectile energies for the measured cross section correspond already to energies below the center of the solar Gamow peak (E0=22 keV). The data provide no evidence for the