We have computed one-nucleon spectroscopic overlaps in light nuclei
by using the Green's function Monte Carlo wave functions.
The realistic Argonne *v _{18}* two-nucleon and Illinois-7
three-nucleon interactions were used to generate the nuclear states.
The overlap functions are used to obtain spectroscopic factors and
asymptotic normalization coefficients, and they can serve as an input
for a variety of reaction calculations.

The *A*=6,7 results given here are for "Type I" wave functions.
For more details, see
I. Brida, S. C. Pieper, and R. B. Wiringa, "Quantum Monte Carlo
calculations of spectroscopic overlaps in *A*≤7 nuclei,"
Phys. Rev. C. **84**, 024319 (2011) or
(arXiv:1106.3121v1 [nucl-th]).

^{7}He(3/2-,g.s.) → ^{6}He(0+,g.s.) + n

^{7}Li(3/2-,g.s.) → ^{6}He(0+,g.s.) + p

^{7}Li(3/2-,g.s.) → ^{6}He(2+) + p

^{7}Li(3/2-,g.s.) → ^{6}Li(1+,g.s.) + n

^{7}Li(3/2-,g.s.) → ^{6}Li(3+) + n

^{7}Li(3/2-,g.s.) → ^{6}Li(0+) + n

^{7}Li(1/2-) → ^{6}Li(1+,g.s.) + n

^{7}Be(3/2-,g.s.) → ^{6}Li(1+,g.s.) + p

^{7}Be(3/2-,g.s.) → ^{6}Li(3+) + p

^{7}Be(3/2-,g.s.) → ^{6}Li(0+) + p

*Ivan Brida*

*Last update 18 June 2014*