In a binary containing a neutron star and an exploding star, hypercritical accretion can push neutron stars past the density threshold for quark deconfinement, forming strange quark stars.
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On the formation of strange quark stars from supernova in compact binaries
In a binary containing a neutron star and an exploding star, hypercritical accretion can push neutron stars past the density threshold for quark deconfinement, forming strange quark stars.