Symbolic regression estimates neutron-star radii from gravitational-wave data alone
A new arXiv preprint explores using symbolic regression to infer neutron-star radii from gravitational-wave signals emitted during binary neutron-star inspirals. Such signals directly constrain component masses and tidal deformabilities, but radii are normally obtained through electromagnetic observations. The approach aims to support multi-messenger studies by deriving radius estimates without relying on electromagnetic data.