Title of article
The image S-factor at solar energies: The prompt γ experiment at LUNA Original Research Article
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 ,
Issue Information
هفته نامه با شماره پیاپی سال 2008
Pages
15
From page
144
To page
158
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
Journal title
Nuclear physics A
Serial Year
2008
Journal title
Nuclear physics A
Record number
1205637
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