Tidal deformability modeling for pulsar companions enables constraints on their equations of state by matching predicted orbital precession to timing data from four systems.
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What Are Pulsar Companions Made of? Using Gravitational Tides to Probe Their Compositions
Tidal deformability modeling for pulsar companions enables constraints on their equations of state by matching predicted orbital precession to timing data from four systems.
- On the Possibility of a Strong First-Order Phase Transition in Neutron Stars