The rate of the hydrogen-burning carbon-nitrogen-oxygen (CNO) cycle is controlled by the slowest process, 14N(p,γ )15O, which proceeds by capture to the ground and several excited states in 15O. Previous extrapolations for the ground state contribution disagreed by a factor 2, corresponding to 15% uncertainty in the total astrophysical S factor. At the Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator placed deep underground in the Gran Sasso facility in Italy, a new experiment on ground state capture has been carried out at 317.8, 334.4, and 353.3 keV center-of-mass energy. Systematic corrections have been reduced considerably with respect to previous studies by using a Clover detector and by adopting a relative analysis. The previous discrepancy has been resolved, and ground state capture no longer dominates the uncertainty of the total S factor.
Precision study of ground state capture in the 14N(p,g)15O reaction / M., Marta; A., Formicola; Gy, Gyurky; D., Bemmerer; C., Broggini; A., Caciolli; P., Corvisiero; H., Costantini; Z., Elekes; Fulop, Z. s.; G., Gervino; A., Guglielmetti; C., Gustavino; Imbriani, Gianluca; M., Junker; R., Kunz; A., Lemut; Limata, BENEDICTA NORMANNA; C., Mazzocchi; R., Menegazzo; P., Prati; Roca, Vincenzo; C., Rolfs; Romano, Mario; C., Rossi Alvarez; E., Somorjai; O., Straniero; F., Strieder; F., Terrasi; H. P., Trautvetter. - In: PHYSICAL REVIEW. C, NUCLEAR PHYSICS. - ISSN 0556-2813. - STAMPA. - 78:2(2008), pp. 022802.1-022802.4. [10.1103/PhysRevC.78.022802]
Precision study of ground state capture in the 14N(p,g)15O reaction
IMBRIANI, GIANLUCA;LIMATA, BENEDICTA NORMANNA;ROCA, VINCENZO;ROMANO, MARIO;
2008
Abstract
The rate of the hydrogen-burning carbon-nitrogen-oxygen (CNO) cycle is controlled by the slowest process, 14N(p,γ )15O, which proceeds by capture to the ground and several excited states in 15O. Previous extrapolations for the ground state contribution disagreed by a factor 2, corresponding to 15% uncertainty in the total astrophysical S factor. At the Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator placed deep underground in the Gran Sasso facility in Italy, a new experiment on ground state capture has been carried out at 317.8, 334.4, and 353.3 keV center-of-mass energy. Systematic corrections have been reduced considerably with respect to previous studies by using a Clover detector and by adopting a relative analysis. The previous discrepancy has been resolved, and ground state capture no longer dominates the uncertainty of the total S factor.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
