Eccentric neutron star–black hole mergers, through their improved parameter measurements, could reveal spin–orbit misalignment and neutron-star mass structure with roughly 2–10 detections in LVK O5.
Maximum mass cutoff in the neutron star mass distribution and the prospect of forming supramassive objects in the double neutron star mergers , volume=
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Eccentricity as a Magnifying Glass: Precision Population Inference Enabled by Eccentric Neutron Star-Black Hole Mergers
Eccentric neutron star–black hole mergers, through their improved parameter measurements, could reveal spin–orbit misalignment and neutron-star mass structure with roughly 2–10 detections in LVK O5.