Neutron star matter from the chiral FRG equation of state behaves as a relativistic Fermi liquid, with extracted Landau parameters F0 and F1 and squared sound speed exceeding 1/3 above about four times nuclear density.
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
-
Neutron Star Matter as a Relativistic Fermi Liquid
Neutron star matter from the chiral FRG equation of state behaves as a relativistic Fermi liquid, with extracted Landau parameters F0 and F1 and squared sound speed exceeding 1/3 above about four times nuclear density.