Asymptotic normalization coefficient for from the reaction and the astrophysical S factor
SV Artemov, R Yarmukhamedov, N Burtebayev… - The European Physical …, 2022 - Springer
This work is aimed at clarifying the contribution of the proton direct radiative capture to the
12 C (p, γ) 13 N reaction by specifying the value of the asymptotic normalization coefficient …
12 C (p, γ) 13 N reaction by specifying the value of the asymptotic normalization coefficient …
Measurement of the keV resonance in the reaction
S Daigle, KJ Kelly, AE Champagne, MQ Buckner… - Physical Review C, 2016 - APS
The N 14 (p, γ) O 15 reaction regulates the power generated by the CN cycle and thus
impacts the structure and evolution of every star at some point in its life. The lowest positive …
impacts the structure and evolution of every star at some point in its life. The lowest positive …
Solar fusion III: New data and theory for hydrogen-burning stars
In stars that lie on the main sequence in the Hertzsprung Russel diagram, like our sun,
hydrogen is fused to helium in a number of nuclear reaction chains and series, such as the …
hydrogen is fused to helium in a number of nuclear reaction chains and series, such as the …
Lifetime measurements of excited states in
The CNO cycle is the main energy source in stars more massive than our Sun, it defines the
energy production and the cycle time that lead to the lifetime of massive stars, and it is an …
energy production and the cycle time that lead to the lifetime of massive stars, and it is an …
[HTML][HTML] Asymptotic normalization coefficients for 11B+ p→ 12C from the 11B (10B, 9Be) 12C reaction and the 11B (p, γ) 12C astrophysical S-factor
SK Sakhiyev, SV Artemov, N Burtebayev, SB Sakuta… - Results in Physics, 2024 - Elsevier
Abstract The 11 B (10 B, 9 Be) 12 C reaction was studied at the energy of 41.3 MeV with
transitions to the ground (0+) and low-lying excited 4.44 MeV (2+) and 9.64 MeV (3−) states …
transitions to the ground (0+) and low-lying excited 4.44 MeV (2+) and 9.64 MeV (3−) states …
Radiative capture of proton through the 14N (p, γ) 15O reaction at low energy
The CNO cycle is the main source of energy in stars more massive than our Sun. This
process defines the energy production, the duration of which can be used to determine the …
process defines the energy production, the duration of which can be used to determine the …
The effect of the 14n (p, γ) 15o reaction on the blue loops in intermediate-mass stars
GM Halabi, MF El Eid, A Champagne - The Astrophysical Journal, 2012 - iopscience.iop.org
We present stellar evolutionary sequences of stars in the mass range 5–12 M☉, having
solar-like initial composition. The stellar models are obtained using updated input physics …
solar-like initial composition. The stellar models are obtained using updated input physics …
Asymptotic theory of charged particle transfer reactions at low energies and nuclear astrophysics
R Yarmukhamedov, KI Tursunmakhatov… - International Journal of …, 2019 - World Scientific
An asymptotic theory is proposed for the peripheral transfer A (x, y) B reaction at low
energies within the three-body (A, a and y) model by combining the dispersion theory and …
energies within the three-body (A, a and y) model by combining the dispersion theory and …
Radiative Capture of proton 14N (p,{\gamma}) 15O at Low Energy
The CNO cycle is the main source of energy in stars more massive than our Sun. It defines
the energy production and the duration contributes in determining the lifetime of massive …
the energy production and the duration contributes in determining the lifetime of massive …
Reaction rate of p capture to all bound states in potential cluster model
S Dubovichenko, N Burkova… - … Journal of Modern …, 2020 - World Scientific
Review of calculation results for astrophysical S-factor of the 1 4 N (p, γ) 1 5 O capture
reaction in the p 1 4 N channel of 1 5 O was presented. It was carried out in the frame of the …
reaction in the p 1 4 N channel of 1 5 O was presented. It was carried out in the frame of the …