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Research Frontiers in Neutron Star Equation of State Constraints

Use of multi-messenger observations including gravitational waves to determine nuclear matter properties at extreme densities.

Gravitational Wave Echoes from Neutron Star Mergers
Quark Matter Phases at Nuclear Density Extremes
Millisecond Pulsar Spin-Down as EOS Probe
X-ray Bursts and the Crust-Core Transition
Tidal Deformability Across the Mass Gap
Hyperon Softening and Maximum Neutron Star Mass
Magnetic Field Effects on Dense Matter Structure
Strangeness Carriers in Superdense Nuclear Matter
Post-Merger Oscillations and Core Composition
Transient Electromagnetic Signatures of Phase Transitions

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