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.
Hadronization in the SU(3) Nambu–Jona-Lasinio model.Phys
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
nucl-th 1years
2019 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
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.