Calculation of the nuclear vertex constant (asymptotic normalization coefficient) for the virtual decay 6Li → α + d on the basis of the three-body model and application of the result in describing the astrophysical …
LD Blokhintsev, SB Igamov, MM Nishonov… - Physics of Atomic …, 2006 - Springer
Within the (α, n, p) three-body model, the s-wave 6 Li→ α+ d vertex constant G 01 and the
asymptotic normalization coefficient C 01 (these two quantities are proportional to each
other) for the wave function describing the 6 Li nucleus in the α+ d channel are calculated by
solving Faddeev equations for various sets of nucleon-nucleon and α N potentials. The
resulting values of G 01 and C 01 are used to calculate the astrophysical factor S (E) for the
radiative-capture reaction d (α, γ) 6 Li at energies in the range E= 0–600 keV. The calculated …
asymptotic normalization coefficient C 01 (these two quantities are proportional to each
other) for the wave function describing the 6 Li nucleus in the α+ d channel are calculated by
solving Faddeev equations for various sets of nucleon-nucleon and α N potentials. The
resulting values of G 01 and C 01 are used to calculate the astrophysical factor S (E) for the
radiative-capture reaction d (α, γ) 6 Li at energies in the range E= 0–600 keV. The calculated …
Calculation of the nuclear vertex constant (asymptotic normalization coefficient) for the virtual decay {sup 6} Li {sup {yields}}{alpha}+ d on the basis of the three-body …
SB Igamov, MM Nishonov, R Yarmukhamedov - Physics of Atomic Nuclei, 2006 - osti.gov
Within the ({alpha}, n, p) three-body model, the s-wave {sup 6} Li {sup {yields}}{alpha}+ d
vertex constant G {sub 01} and the asymptotic normalization coefficient C {sub 01}(these two
quantities are proportional to each other) for the wave function describing the {sup 6} Li
nucleus in the {alpha}+ d channel are calculated by solving Faddeev equations for various
sets of nucleon-nucleon and {alpha} N potentials. The resulting values of G {sub 01} and C
{sub 01} are used to calculate the astrophysical factor S (E) for the radiative-capture reaction …
vertex constant G {sub 01} and the asymptotic normalization coefficient C {sub 01}(these two
quantities are proportional to each other) for the wave function describing the {sup 6} Li
nucleus in the {alpha}+ d channel are calculated by solving Faddeev equations for various
sets of nucleon-nucleon and {alpha} N potentials. The resulting values of G {sub 01} and C
{sub 01} are used to calculate the astrophysical factor S (E) for the radiative-capture reaction …
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