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Understanding how matter behaves at the highest densities and temperatures isa major open problem in both nuclear physics and relativistic astrophysics.This physics is often encapsulated in the so-called high-temperature nuclearequation of state, which influences compact binary mergers, core-collapsesupernovae, and many more phenomena. One such case is the type (either blackhole or neutron star) and mass of the remnant of the core collapse of a massivestar. For each of six candidate equations of state, we use a very large suiteof spherically symmetric supernova models to generate a suite of syntheticpopulations of such remnants. We then compare these synthetic populations tothe observed remnant population. We thus provide a novel constraint on thehigh-temperature nuclear equation of state and describe which EOS candidatesare more or less favored by this metric.

A New Constraint on the Nuclear Equation of State from Statistical Distributions of Compact Remnants of Supernovae