Matching the crust and core equations of state with different smooth interpolation functions has only a modest effect on the predicted mass, radius, and tidal deformability of neutron stars, provided the matching occurs above the crust-core transition.
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
CONDITIONAL 1representative citing papers
citing papers explorer
-
An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars
Matching the crust and core equations of state with different smooth interpolation functions has only a modest effect on the predicted mass, radius, and tidal deformability of neutron stars, provided the matching occurs above the crust-core transition.