A chameleon-Kiselev neutron star model claims scalar-driven pressure anisotropies, a 1.75 solar mass maximum, and an 86% tidal deformability suppression, but headline numbers contradict each other across the paper.
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Quintessence-Chameleon transitions in anisotropic Kiselev model of neutron stars
A chameleon-Kiselev neutron star model claims scalar-driven pressure anisotropies, a 1.75 solar mass maximum, and an 86% tidal deformability suppression, but headline numbers contradict each other across the paper.