The rate at which helium (He 4) and deuterium (d) fuse together to produce lithium-6 (Li 6)
and a γ ray, He 4 (d, γ) Li 6, is a critical puzzle piece in resolving the discrepancy between …

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 …

At the long-wavelength approximation, E1 transitions are forbidden between isospin-zero
states. Hence E1 radiative capture is strongly hindered in reactions involving N= Z nuclei but …

The astrophysical S factor and reaction rate of the direct capture process α+ d→ Li 6+ γ, as
well as the abundance of the Li 6 element, are estimated in a three-body model. The initial …

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 …

Radiative capture reaction d (α, γ) 6 L id(α,γ)^6Li is the only process in the Big-Bang model
that produces L 6 i ^6Li. We develop the formalism based on pionless Effective Field Theory …

The astrophysical He 3 (α, γ) Be 7 and H 3 (α, γ) Li 7 direct capture processes are studied in
the framework of the two-body model with potentials of a simple Gaussian form, which …

The α+ d→ 6 Li+ γ radiative capture is studied in order to predict the Li 6 primordial
abundance. Within a two-body framework, the α particle and the deuteron are considered …

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 …