A hybrid neutron star model with an intermediate hypernuclear shell and a stiff color-superconducting quark core can reach 2.2 solar masses and satisfies current mass and radius constraints.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
nucl-th 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
First-order phase transition from hypernuclear matter to deconfined quark matter obeying new constraints from compact star observations
A hybrid neutron star model with an intermediate hypernuclear shell and a stiff color-superconducting quark core can reach 2.2 solar masses and satisfies current mass and radius constraints.