The astrophysical rate of 15O(alpha,gamma)19Ne via the (p,t) reaction in inverse kinematics
B. Davids, A. M. van den Berg, P. Dendooven, F. Fleurot, M. Hernanz, M. Hunyadi, M. A. de Huu, J. Jose, K. E. Rehm, R. E. Segel, R. H. Siemssen, H. W. Wilschut, H. J. Wortche, A. H. Wuosmaa
Abstract
A recoil coincidence technique has been applied to measure the alpha-decay branching ratios of near-threshold states in 19Ne. Populating these states using the (p,t) reaction in inverse kinematics, we detected the recoils and their decay products with 100% geometric efficiency using a magnetic spectrometer. Combining our branching ratio measurements with independent determinations of the radiative widths of these states, we calculate the astrophysical rate of 15O(alpha,gamma)19Ne. Using this reaction rate, we perform hydrodynamic calculations of nova outbursts and conclude that no significant breakout from the hot CNO cycles into the rp process occurs in novae via 15O(alpha,gamma)19Ne.
Create a lesson
Related papers
Probing high-momentum components in 16O via zero-degree (p,d) cross-section ratios
FRS Experiment Collaboration, X. Wang, H. J. Ong et al.
Double-differential neutron-induced cross sections on Fe-nat at GANIL-NFS
L. de Arruda, D. Tarrío, X. Ledoux et al.
Event-by-event net-charge fluctuations in pp, OO, Ne-Ne, and Pb-Pb collisions with ALICE at the LHC
Nida Malik
Charge exchange reactions with central and tensor interactions and nuclear matrix elements associated with double-beta-decay neutrinos and astro neutrinos
Hiroyasu Ejiri, Yoritaka Iwata
First Measurement of Compton Scattering on 3He at HIγS
J. Zhou, E. Mancil, M. W. Ahmed et al.
Evolution of high-spin states in neutron-rich 195-202Au isotopes approaching the N=126 shell closure
Y. Cho, Y. H. Kim, A. Navin et al.