Other
Scientific paper
Apr 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aps..aprj13008a&link_type=abstract
American Physical Society, APS April Meeting, April 16-19, 2005, abstract #J13.008
Other
Scientific paper
Data from γ-ray space telescopes suggest that ^22Na is under produced in ONe novae compared to model calculations. This could be explained if the parent ^22Mg is depleted by the ^22Mg(p,γ)^23Al reaction. We are determining the asymptotic normalization coefficients (ANCs) for ^23Al->^22Mg+p to estimate this reaction rate. The neutron transfer reaction ^13C(^22Ne,^23Ne)^12C, θC.M =3^o-34^o, was measured using a 264 MeV ^22Ne beam from the Texas A&M K500 cyclotron to extract the ANCs for the ground and first excited states in ^23Ne, and then transpose to the corresponding states of the mirror nucleus ^23Al. Another experiment was carried out to obtain the ANC for ^13C->^12C+n, θC.M =3^o-38^o, which is the other vertex in the above reaction. Elastic scattering angular distributions for both reactions were also measured to obtain reliable optical potential parameters that will be used in DWBA calculations. New results will be presented and discussed.
Al-Abdullah Tariq
Carstoiu Florin
Piskoř Š.
No associations
LandOfFree
Extracting the ANCs for ^23Al->^22Mg + p from the mirror system ^23Ne->^22Ne + n does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Extracting the ANCs for ^23Al->^22Mg + p from the mirror system ^23Ne->^22Ne + n, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extracting the ANCs for ^23Al->^22Mg + p from the mirror system ^23Ne->^22Ne + n will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1454914