Microscopic chiral-EFT equation of state for beta-stable neutron matter yields tidal deformability values inside GW170817 bounds and excludes stiff EOS with radii above ~13 km.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
nucl-th 1years
2025 1verdicts
UNVERDICTED 1representative citing papers
citing papers explorer
-
Tidal deformability in neutron stars from a microscopic point of view
Microscopic chiral-EFT equation of state for beta-stable neutron matter yields tidal deformability values inside GW170817 bounds and excludes stiff EOS with radii above ~13 km.