The H (α, γ) 2 Li 6 radiative capture responsible for the Li 6 production during the big-bang
nucleosynthesis is comprehensively studied within a microscopic approach. The approach …

Astrophysical S factors and reaction rates of the direct radiative capture processes He 3 (α,
γ) 7 Be and H 3 (α, γ) 7 Li, as well as the primordial abundance of the Li 7 element, are …

Reaction rate of the process d (α, γ) 6 Li has been calculated in the framework of Effective
Field Theory (EFT) at low energy. Deuteron is assumed as a dibaryon in the initial state. The …

Two of the main components of nuclear fusion processes which occur in stars are the
radiative capture of deuteron-alpha and its inverse reaction during which helium transforms …

The D (p, γ) He 3 reaction, where 'D'denotes 'H 2', is of primary importance in cosmology and
nuclear physics since it offers a unique opportunity to test predictions based on the …

The astrophysical S factor and reaction rates of the direct capture process Li 6 (p, γ) Be 7 are
estimated within a two-body single-channel potential model approach. Nuclear potentials of …

The H six-nucleon system is studied within a microscopic cluster approach formulated in the
oscillator-basis representation. The total and partial astrophysical factors for the radiative …

Nuclear reaction theory is important, especially at low energies, as are predictions of the
characteristics of the heaviest nuclei, including processes for laboratory synthesis, and …

An infinity of extensions of the Siegert transformation exist in the Coulomb gauge. All
resulting transition multipoles of the electric field are identical at the long-wavelength …

Astrophysical S-factors at zero energy for the direct nuclear capture reactions $^{3}{\rm
He}(\alpha,\gamma)^{7}{\rm Be} $, $^{3}{\rm H}(\alpha,\gamma)^{7}{\rm Li} $ and $^{7}{\rm …