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Chandrasekhar limit

White dwarfs can turn into neutron stars under certain conditions

White dwarfs can turn into neutron stars under certain conditions

September 16, 2026 by Sophie Lin - Technology Editor

This evolutionary pathway is known as accretion-induced collapse, a process where the stellar remnant accumulates matter transferred to it by a companion star.

Categories Technology Tags accretion-induced collapse, Chandrasekhar limit, ETH Zurich, Laurenz Tümmler, neutron star formation, oxygen-neon-magnesium white dwarfs, Type Ia supernova Leave a comment

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