105 citations · 557 across the 13 of their papers we have counts for
13 papers
Bayesian Smooth-Fit Extrapolation of the Astrophysical Factor
A. M. Mukhamedzhanov
A Bayesian analysis of the astrophysical \(S\) factor for the \(^{12}{\rm C}+{}^{12}{\rm C}\) fusion reaction is presented using available low-energy information at carbon--carbon…
Bayesian Framework for the E1 and E2 Astrophysical Factors at 300 keV from Subthreshold and Ground-State Asymptotic Normalization Coefficients
A. M. Mukhamedzhanov
The reaction governs the carbon-to-oxygen ratio set during helium burning, shaping white-dwarf structure and Type~Ia supernova yields. At the…
Asymptotic normalization coefficients for synthesis and the -factor for radiative capture
A. M. Mukhamedzhanov, R. J. deBoer, B. F. Irgaziev +3
The O reaction, determining the survival of carbon in red giants, is of interest for nuclear reaction theory and nuclear astrophysics. A specific feature of…
Constraining the 6.05 MeV 0 and 6.13 MeV 3 cascade transitions in the C(,)O reaction using the Asymptotic Normalization Coefficients
M. L. Avila, G. V. Rogachev, E. Koshchiy +7
Background. The CO reaction plays a fundamental role in astrophysics and needs to be known with accuracy better than 10%. Cascade transitions through the exc…
Astrophysical S factor for the radiative capture 12N(p,gamma)13O determined from the 14N(12N,13O)13C proton transfer reaction
A. Banu, T. Al-Abdullah, C. Fu +10
The cross section of the radiative proton capture reaction on the drip line nucleus 12N was investigated using the Asymptotic Normalization Coefficient (ANC) method. We have used t…
Astrophysical factor for the neutron generator 13C(alpha,n)16O reaction in the AGB stars
E. D. Johnson, G. V. Rogachev, A. M. Mukhamedzhanov +15
The reaction 13C(alpha,n) is considered to be the main source of neutrons for the s-process in AGB stars. At low energies the cross section is dominated by the 1/2+ 6.356 MeV sub-t…