Effective models indicate the hadron-quark pasta phase occurs only in very massive, slowly rotating neutron stars below ~300 Hz, while the 't Hooft term produces noticeable shifts in hot hadron-quark star composition.
Phase diagram of three-flavor quark matter under compact star constraints
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Phases of Hadron-Quark Matter in (Proto) Neutron Stars
Effective models indicate the hadron-quark pasta phase occurs only in very massive, slowly rotating neutron stars below ~300 Hz, while the 't Hooft term produces noticeable shifts in hot hadron-quark star composition.