The astrophysical S factors of E1 and E2 capture data of 12C( α , γ) reaction at 300 keV have been calculated based on our recent determined ANC values of 6.92 MeV and 7.12 MeV states of 16O using R-matrix. The S-factors are extrapolated into the range of burning temperature and the S-factors at 300 keV are S E1= (86 ± 34) keV b and SE2= (60 ± 33) keV b
The ¹²C(α,γ)¹⁶O reaction, an important component of stellar helium burning, has a key role in nuclea...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
The astrophysical S factors of E1 and E2 capture data of 12C( α , γ) reaction at 300 keV have been c...
The radiative capture cross sections of 12C(α,γ)16O and derived reaction rates are calculated from t...
The 12C(α, γ)16O reaction plays a key role in the evolution of stars with masses of M > 0.55 M⊙. At ...
The astrophysical S-factors of the 13C(α,n) 16O17O(α,n) 20Ne21Ne(α,n) 24Mg and 25Mg(α,n) 28Si reacti...
Because of the critical importance of the ^(12)/^(16)O ratio resulting from helium burning to the la...
The cross section for the reaction ^(12)C(α, γ)^(16)O has been measured for a range of c.m. energies...
The cross section for the reaction ^(12)C(α, γ)^(16)O has been measured for a range of c.m. energies...
The most recent data for the 12C(α,γ)16O reaction are parametrized in terms of a K matrix in order t...
The cross section for the reaction ^(12)C(α, γ)^(16)O has been measured for a range of c.m. energies...
A new measurement of the β-delayed α decay of N16 has been performed using a set of high efficiency ...
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
The ¹²C(α,γ)¹⁶O reaction, an important component of stellar helium burning, has a key role in nuclea...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
The astrophysical S factors of E1 and E2 capture data of 12C( α , γ) reaction at 300 keV have been c...
The radiative capture cross sections of 12C(α,γ)16O and derived reaction rates are calculated from t...
The 12C(α, γ)16O reaction plays a key role in the evolution of stars with masses of M > 0.55 M⊙. At ...
The astrophysical S-factors of the 13C(α,n) 16O17O(α,n) 20Ne21Ne(α,n) 24Mg and 25Mg(α,n) 28Si reacti...
Because of the critical importance of the ^(12)/^(16)O ratio resulting from helium burning to the la...
The cross section for the reaction ^(12)C(α, γ)^(16)O has been measured for a range of c.m. energies...
The cross section for the reaction ^(12)C(α, γ)^(16)O has been measured for a range of c.m. energies...
The most recent data for the 12C(α,γ)16O reaction are parametrized in terms of a K matrix in order t...
The cross section for the reaction ^(12)C(α, γ)^(16)O has been measured for a range of c.m. energies...
A new measurement of the β-delayed α decay of N16 has been performed using a set of high efficiency ...
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
New data on the spectrum of α particles following the 16N β decay are used to revise and extend a pr...
The ¹²C(α,γ)¹⁶O reaction, an important component of stellar helium burning, has a key role in nuclea...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...
The E1 astrophysical S factor for the 12C(α,γ)16O reaction is studied using R-matrix theory. The con...