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Measurement of the 3He(3He,2p)4He cross section within the solar Gamow peak

✍ Scribed by C. Arpesella; E. Bellotti; C. Broggini; P. Corvisiero; G. Fiorentini; A. Fubini; G. Gervino; U. Greife; C. Gustavino; M. Junker; J. Lambert; P. Prati; W.S. Rodney; C. Rolfs; H.P. Trautvetter; D. Zahnow; S. Zavatarelli


Book ID
108439082
Publisher
Elsevier Science
Year
1996
Tongue
English
Weight
330 KB
Volume
389
Category
Article
ISSN
0370-2693

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πŸ“œ SIMILAR VOLUMES


The cross section of 3He(3He,2p)4He meas
✍ M. Junker; C. Arpesella; E. Bellotti; C. Broggini; P. Corvisiero; A. D'Alessandr πŸ“‚ Article πŸ“… 1999 πŸ› Elsevier Science 🌐 English βš– 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

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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, Ξ³) 3 He cross section from 22 down to