A self-consistent constant-density star solution with quantum trace-anomaly backreaction is found, whose parameter space contains ultra-compact configurations arbitrarily close to the Schwarzschild limit.
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Self-consistent solution to the semiclassical Einstein equations of a star
A self-consistent constant-density star solution with quantum trace-anomaly backreaction is found, whose parameter space contains ultra-compact configurations arbitrarily close to the Schwarzschild limit.