Enhanced Nuclear Binding Near the Proton Dripline Opens Possible Bypass of the $^{64}{\rm Ge}$ rp-process Waiting Point

We performed astrophysics model calculations with updated nuclear data to identify a possible bypass of the $^{64}{\rm Ge}$ waiting-point, a defining feature of the rapid-proton capture (rp-) process that powers type-I x-ray bursts on accreting neutron stars. We find that the rp-process flow through the $^{64}{\rm Ge}$ bypass could be up to 36\% for astrophysically relevant conditions. Our results call for new studies of $^{65}{\rm Se}$, including the nuclear mass, $β$-delayed proton emission branching, and nuclear structure as it pertains to the $^{64}{\rm As}(p,γ)$ reaction rate at x-ray burst temperatures.