G. Grinyer

Model-observation comparisons of type-I X-ray bursts (XRBs) can reveal the properties of accreting neutron star systems, including the neutron star compactness. XRBs are powered by…

nucl-ex2025

Unbound neutron $ν 0 d_{3/2}$ strength in $^{17}$ C and the N=16 shell gap

J. Lois-Fuentes, B. Fernández-Domínguez, F. Delaunay +61

Significant continuum strength has been observed to be populated in $^{17}$ C produced in the d( $^{16}$ C,p) reaction at a beam energy of 17.2~MeV/nucleon. The strength appears at gr…

Direct measurement of 59Cu(p,α)56Ni precludes a strong NiCu cycle in Type-I X-ray bursts

Unbound neutron ν0d3/2​ strength in 17C and the N=16 shell gap

Direct measurement of $^{59}$ Cu( $p$ , $α$ ) $^{56}$ Ni precludes a strong NiCu cycle in Type-I X-ray bursts

Unbound neutron $ν 0 d_{3/2}$ strength in $^{17}$ C and the N=16 shell gap