Cold r-process in neutrino-driven winds

The r-process in a low-temperature environment is explored, in which the neutron emission by photodisintegration does not play a role (cold r-process). A semianalytic neutrino-driven wind model is utilized for this purpose. The temperature in a supersonically expanding outflow can quickly drop to a few K, where the 8 10 (n,gamma)-(gamma,n) equilibrium is never achieved during the heavy r-nuclei synthesis. In addition, the neutron capture n, g g, n competes with the beta-decay owing to the low matter density. Despite such nonstandard physical conditions for the cold r-process, a solar-like r-process abundance curve can be reproduced. The cold r-process predicts, however, low lead production compared to that expected in the traditional r-process conditions, which can be a possible explanation for the low lead abundances found in a couple of r-process-rich Galactic halo stars.