Indirect methods of determination of the asymptotic normalization coefficients and their application for nuclear astrophysics

2014 ◽  
Author(s):  
R. Yarmukhamedov
2014 ◽  
Vol 64 (4) ◽  
pp. 461-472 ◽  
Author(s):  
V. V. Karpov ◽  
I. B. Polovov ◽  
D. Kudryashov ◽  
D. G. Lisienko ◽  
V. A. Volkovich ◽  
...  

1985 ◽  
Vol 111 ◽  
pp. 459-461
Author(s):  
L. Pastori ◽  
L. E. Pasinetti ◽  
E. Antonello

Several direct and indirect methods for the determination of stellar apparent diameters have been developed in the past; they are summarized in Table 1 by Fracassini, et al. (1981) with a code number and references. So far, no detailed comparison of the methods has been carried out, the main difficulty being the extremely small number of common stars. Nevertheless, from the stars listed in CADARS (Fracassini, et al. 1981), we have obtained some correlations in order to test the reliability of some methods and to define the regions of the HR diagram where they can be applied.


2003 ◽  
Vol 719 ◽  
pp. C119-C122 ◽  
Author(s):  
V. Kroha ◽  
A. Azhari ◽  
P. Bém ◽  
V. Burjan ◽  
C.A. Gagliardi ◽  
...  

2018 ◽  
Vol 184 ◽  
pp. 01014
Author(s):  
J. Mrazek ◽  
V. Burjan ◽  
V. Kroha ◽  
A.M. Mukhamedzhanov ◽  
R. Tribble ◽  
...  

Asymptotic Normalization Coefficients method is one of the indirect methods used in nuclear astrophysics. The method allows to deduce a direct part of a radiative capture cross section from the measurement of a two body reaction under specific conditions. The experimental works started in collaboration of NPI CAS, TAMU and INFN LNS from 90-ties and continue till the present. The introduction to this method is presented and experimental experiences from NPI CAS and the collaboration are shared.


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