Indirect techniques in nuclear astrophysics: a review

RE Tribble, CA Bertulani, M La Cognata… - Reports on Progress …, 2014 - iopscience.iop.org
In this review, we discuss the present status of three indirect techniques that are used to
determine reaction rates for stellar burning processes, asymptotic normalization coefficients …

New theoretical results for radiative , , and captures at astrophysical energies

S Dubovichenko… - … Journal of Modern …, 2019 - World Scientific
We have studied the proton capture reaction 3 H (p, γ) 4 He. It plays a role in the
nucleosynthesis of primordial elements in the early Universe leading to the prestellar …

Astrophysical S-factor for the 3He (α, γ) 7Be reaction via the asymptotic normalization coefficient (ANC) method

GG Kiss, M La Cognata, C Spitaleri… - Physics Letters B, 2020 - Elsevier
The detection of the neutrinos produced in the p− p chain and in the CNO cycle can be used
to test the Standard Solar Model. The 3 He (α, γ) 7 Be reaction is the first reaction of the 2nd …

Indirect determination of the astrophysical factor for the ( reaction using the asymptotic normalization coefficient method

GG Kiss, M La Cognata, R Yarmukhamedov… - Physical Review C, 2021 - APS
Background: The Li 6 (p, γ) Be 7 cross section influences a variety of astrophysical
scenarios, including big-bang and stellar nucleosynthesis. In recent years, conflicting results …

and nuclei within the no-core shell model with continuum

M Vorabbi, P Navrátil, S Quaglioni, G Hupin - Physical Review C, 2019 - APS
Background: The production of Be 7 and Li 7 nuclei plays an important role in primordial
nucleosynthesis, nuclear astrophysics, and fusion energy generation. The He 3 (α, γ) Be 7 …

New measurements of the astrophysical S factor for 12 C (p, γ) 13 N reaction at low energies and the asymptotic normalization coefficient (nuclear vertex constant) for …

N Burtebaev, SB Igamov, RJ Peterson… - Physical Review C …, 2008 - APS
New measurements of differential and total cross sections for the 12 C (p, γ) 13 N reaction
have been made at beam energies of E p= 354, 390, 460, 463, 565, 750, and 1061 keV …

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 …

Astrophysical S factors of reactions with light nuclei

SB Dubovichenko, YN Uzikov - Physics of Particles and Nuclei, 2011 - Springer
The two-cluster model is a phenomenological semi-microscopic approach to the study of
multinucleon nuclear systems. In the framework of this model, interaction of nucleon clusters …

Low-energy bound states, resonances, and scattering of light ions

BK Luna, T Papenbrock - Physical Review C, 2019 - APS
We describe bound states, resonances, and elastic scattering of light ions using a δ-shell
potential. Focusing on low-energy data such as energies of bound states and resonances …

Asymptotic normalization coefficients for from the peripheral reaction and their astrophysical application

OR Tojiboev, R Yarmukhamedov, SV Artemov… - Physical Review C, 2016 - APS
The proton transfer Be 7 (d, n) B 8 reaction at the energy of 4.5 MeV (center of mass) has
been analyzed within the modified distorted-wave Born approximation. New estimates and …