Cole Miller's research in the last few years has focused on theory and modeling of high-energy radiation from neutron stars and black holes. Data interpreted using his theoretical models have provided the first evidence for the existence of an innermost stable circular orbit around neutron stars and black holes (a key prediction of strong-gravity general relativity) and evidence for a 2.3 solar mass neutron star, which constrains strongly the equation of state of matter at high densities.

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