space.com
The universe’s most extreme dead stars can form from vampire white dwarfs — and scientists finally know how
A recent study by ETH Zurich researchers has mapped the precise conditions under which a white dwarf can collapse into a neutron star through accretion‑induced collapse (AIC). The process requires a white dwarf composed of oxygen, neon, and magnesium, which are denser and more massive than typical carbon‑oxygen white dwarfs. The star must accrete material from a companion at a rate that brings it close to the Chandrasekhar limit without exceeding it, preventing a Type Ia supernova. AIC [...]