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nucl-th2026
Coexistence of strange quark stars and neutron stars: metastability and nucleation in proto-neutron stars
Mirco Guerrini, Giuseppe Pagliara, Luca Passarella +1
If strange quark matter (SQM) is absolutely stable, hadronic neutron stars (NSs) and strange quark stars (QSs) may coexist in the so-called two-families scenario. A key issue is ex…
nucl-th2026
Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis
Luca Passarella, Mirco Guerrini, Giuseppe Pagliara +2
Hadronic stars and strange quark stars could coexist within the so-called two-families scenario. In this respect, hadronic matter and strange quark matter correspond to two distinc…
nucl-th2025
Relativistic mean-field predictions for dense matter equation of state and application to neutron stars
Luca Passarella, Jerome Margueron, Giuseppe Pagliara
Relativistic mean-field models (RMF) based on the exchange of , , and mesons including non-linear nucleon- couplings and density-dependent coupling, are considered…