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Observable Signatures of a Quarkyonic Phase in Neutron Stars
Probit J Kalita, Tuhin Malik, Tianqi Zhao +2
Quarkyonic matter in \(β\)-equilibrium is a potential description of cold dense matter in neutron stars (NSs), that introduces non-interacting quarks alongside nucleons and leptons…
Compiled Properties of Nucleonic Matter and Nuclear and Neutron Star Models from Non-Relativistic and Relativistic Interactions
Boyang Sun, Saketh Bhattiprolu, James M. Lattimer
This paper compiles the model parameters and zero-temperature properties of an extensive collection of published theoretical nuclear interactions, including 255 non-relativistic (S…
Constraints on the Nuclear Symmetry Energy from Experiments, Theory and Observations
James M. Lattimer
Nuclear mass measurements and neutron matter theory tightly constrain the nuclear symmetry energy parameters , , and . Corroboration of these constraints o…
Constraints on Nuclear Symmetry Energy Parameters
James M. Lattimer
A review is made of constraints on the nuclear symmetry energy parameters arising from nuclear binding energy measurements, theoretical chiral effective field predictions of neutro…
Long Range Plan: Dense matter theory for heavy-ion collisions and neutron stars
Alessandro Lovato, Travis Dore, Robert D. Pisarski +61
Since the release of the 2015 Long Range Plan in Nuclear Physics, major events have occurred that reshaped our understanding of quantum chromodynamics (QCD) and nuclear matter at l…
Limiting masses and radii of neutron stars and their implications
Christian Drischler, Sophia Han, James M. Lattimer +3
We combine equation of state of dense matter up to twice nuclear saturation density () obtained using chiral effective field theory (EFT), and…