Author/Authors :
H. Costantini، نويسنده , , D. Bemmerer، نويسنده , , F. Confortola، نويسنده , , A. Formicola، نويسنده , , Gy. Gyurky، نويسنده , , P. Bezzon، نويسنده , , R. Bonetti، نويسنده , , C. Broggini، نويسنده , , P. Corvisiero، نويسنده , , Z. Elekes، نويسنده , , Zs. Fulop، نويسنده , , G. Gervino، نويسنده , , A. Guglielmetti، نويسنده , , C. Gustavino، نويسنده , , G. Imbriani، نويسنده , , M. Junker، نويسنده , , M. Laubenstein، نويسنده , , A. Lemut، نويسنده , , B. Limata، نويسنده , , V. Lozza، نويسنده , , et al.، نويسنده ,
Abstract :
The View the MathML source process is a key reaction in both Big-Bang nucleosynthesis and p–p chain of Hydrogen Burning in Stars. A new measurement of the View the MathML source cross section has been performed at the INFN Gran Sasso underground laboratory by both the activation and the prompt γ detection methods. The present work reports full details of the prompt γ detection experiment, focusing on the determination of the systematic uncertainty. The final data, including activation measurements at LUNA, are compared with the results of the last generation experiments and two different theoretical models are used to obtain the S-factor at solar energies.
Keywords :
Measured , I? , ? , Branching ratio , deduced , Prompt ? texhnique , HPGe detector in the Gran Sasso undreground laboratory , Comparison with other data , Nuclear reactions , View the MathML source , E=220 , 250 , E? , 400 keV , Astrophysical S-factor
