Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope
This paper proposes a method using third-generation gravitational-wave detectors (Cosmic Explorer and Einstein Telescope) to measure the fractional contribution of binary neutron star mergers to cosmic r-process nucleosynthesis by analyzing the redshift-dependent correlation between merger event rates and r-process abundances, achieving a precision of approximately 5–6% for both multi-messenger "bright-sirens" and "dark-sirens" scenarios.