scholarly journals Connection between effective-range expansion and nuclear vertex constant or asymptotic normalization coefficient

2011 ◽  
Vol 84 (2) ◽  
Author(s):  
R. Yarmukhamedov ◽  
D. Baye
Keyword(s):  
Range Expansion ◽  
Effective Range ◽  
Effective Range Expansion ◽  
Asymptotic Normalization ◽  
Vertex Constant ◽  
Asymptotic Normalization Coefficient

Effective range expansion revisited

1982 ◽  
Vol 119 (4-6) ◽  
pp. 245-248 ◽  
Author(s):  
Sadhan K. Adhikari ◽  
JoséR.A. Torreão
Keyword(s):  
Range Expansion ◽  
Effective Range ◽  
Effective Range Expansion

Updating the effective range expansion of low-energyN $$\bar N$$ -scattering

1991 ◽  
Vol 338 (1) ◽  
pp. 111-112 ◽  
Author(s):  
H. J. Pirner ◽  
B. Kerbikov ◽  
J. Mahalanabis
Keyword(s):  
Range Expansion ◽  
Effective Range ◽  
Effective Range Expansion

scholarly journals Improved effective range expansion for Casimir–Polder potential

2019 ◽  
Vol 73 (12) ◽  
Author(s):  
Pierre-Philippe Crépin ◽  
Romain Guérout ◽  
Serge Reynaud
Keyword(s):  
Range Expansion ◽  
Effective Range ◽  
Effective Range Expansion

scholarly journals Determination of the asymptotic normalization coefficient (nuclear vertex constant) for α + d →6Li from the new direct measured d(α,γ)6Li data and its implication for extrapolating the d(α,γ)6Li astrophysical S factor at Big Bang energies

2019 ◽  
Vol 49 ◽  
pp. 1960017
Author(s):  
K. I. Tursunmakhatov ◽  
R. Yarmukhamedov
Keyword(s):  
Potential Method ◽  
Big Bang ◽  
Asymptotic Normalization ◽  
Vertex Constant ◽  
Asymptotic Normalization Coefficient ◽  
S Factor ◽  
Low Energies ◽  
Body Potential

The results of the analysis of the new experimental astrophysical S factors [Formula: see text] [D. Trezzi et al., Astropart. Phys. 89, 57 (2017)] and those measured earlier [R. G. Robertson et al., Phys. Rev. Lett. 47, 1867 (1981)] for the nuclear-astrophysical [Formula: see text] reaction directly measured at extremely low energies [Formula: see text], which is derived within the modified two-body potential method, are presented. New estimates and their uncertainties have been obtained for values of the asymptotic normalization coefficient for [Formula: see text] and for the direct astrophysical [Formula: see text] factors at Big Bang energies.

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