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Astrophysical implications of the new measurements of the 3He(3He,2p)4He cross section

✍ Scribed by D. Galli; P.G. Prada Moroni; S. Zavatarelli; F. Ferrini; F. Palla

Publisher
Elsevier Science
Year
2001
Tongue
English
Weight
154 KB
Volume
688
Category
Article
ISSN
0375-9474

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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