In 1998, [2] pointed out the big difference for the ('old' experimental data) when experimental results were grouped starting from the main two methods: for the direct capture and for the activation. Its importance for the Standard Solar Model was the reason to ask for new measurements to understand the discrepancy. 'New' results [4]solved this issue by equalizing the above values, but introduced a new situation to clarify: a discrepancy between the variations for 'old' and 'new' data at higher energies than . 'Old' theoretical models, used for extrapolating the to the stellar energies, couldn't explain this new behavior. New experimental data [3, 5] was required, again, by theorists. We started this project with the main goal to clarify the situation. Here are the results.
Skip Nav Destination
Article navigation
20 October 2012
NUCLEAR STRUCTURE AND DYNAMICS 2012
9–13 July 2012
Opatija, Croatia
Research Article|
October 20 2012
astrophysical factor study using activation method
C. Bordeanu
C. Bordeanu
Institute of Nuclear Research (ATOMKI), H-4001 Debrecen, POB.51.,
Hungary
Search for other works by this author on:
AIP Conf. Proc. 1491, 281–284 (2012)
Citation
C. Bordeanu; astrophysical factor study using activation method. AIP Conf. Proc. 20 October 2012; 1491 (1): 281–284. https://doi.org/10.1063/1.4764257
Download citation file:
Sign in
Don't already have an account? Register
Sign In
You could not be signed in. Please check your credentials and make sure you have an active account and try again.
Sign in via your Institution
Sign in via your InstitutionPay-Per-View Access
$40.00
6
Views
Citing articles via
Related Content
β-delayed α decay of 16 N and the 12 C (α,γ) 16 O cross section at astrophysical energies: A new experimental approach
AIP Conference Proceedings (February 2015)
The S E 1 factor of the 12 C (α,γ) 16 O Reaction and the 16 N β‐delayed α Decay
AIP Conference Proceedings (January 2008)
Comparison of B, BF 2 & B 18 H 22 for Extension and BF 2 , B 18 H 22 & In HALO Implantation for 32 nm Node Using Various Diffusion‐less Annealing Techniques
AIP Conference Proceedings (November 2008)
Recent results at LUNA, using a solid target
AIP Conference Proceedings (April 2006)
Recent Astrophysical Experiments on Cyclotron of NPI at Řež in Collaboration with Texas A&M University
AIP Conference Proceedings (January 2008)