Quantum vacuum backreaction in the Polyakov approximation removes the classical horizon from Einstein-Yang-Mills black holes, replacing it with a wormhole for large horizons and a compact horizonless object for small ones.
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Quantum corrected Einstein-Yang-Mills black holes in semiclassical gravity
Quantum vacuum backreaction in the Polyakov approximation removes the classical horizon from Einstein-Yang-Mills black holes, replacing it with a wormhole for large horizons and a compact horizonless object for small ones.