G. Raimann

most citedAstrophysical Reaction Rates for

^{10}

B(p,

α

)

^{7}

Be and

^{11}

B(p,

α

)

^{8}

Be From a Direct Model

36 citations · 63 across the 2 of their papers we have counts for

collaborators

2 papers

nucl-th1996★ 36 cited

Astrophysical Reaction Rates for $^{10}$ B(p, $α$ ) $^{7}$ Be and $^{11}$ B(p, $α$ ) $^{8}$ Be From a Direct Model

T. Rauscher, G. Raimann

The reactions $^{10}$ B(p, $α$ ) $^{7}$ Be and $^{11}$ B(p, $α$ ) $^{8}$ Be are studied at thermonuclear energies using DWBA calculations. For both reactions, transitions to the ground state…

nucl-ex1995★ 27 cited

Study of the levels in $^{17}$ C above the $^{16}$ C + neutron threshold

G. Raimann, A. Ozawa, R. N. Boyd +9

The $β$ -delayed neutron decay of $^{17}$ B was studied using a radioactive ion beam. The neutron energies, measured via time-of-flight, give information on states in $^{17}$ C above…

Astrophysical Reaction Rates for 10B(p,α)7Be and 11B(p,α)8Be From a Direct Model

Study of the levels in 17C above the 16C + neutron threshold

Astrophysical Reaction Rates for $^{10}$ B(p, $α$ ) $^{7}$ Be and $^{11}$ B(p, $α$ ) $^{8}$ Be From a Direct Model

Study of the levels in $^{17}$ C above the $^{16}$ C + neutron threshold