Understand
We present a class of exact analytic and static, spherically symmetric black hole solutions in the semi-classical Einstein equations with Weyl anomaly.
- The solutions have two branches, one is asymptotically flat and the other asymptotically de Sitter.
- We study thermodynamic properties of the black hole solutions and find that there exists a logarithmic correction to the well-known Bekenstein-Hawking area entropy.
- The logarithmic term might come from non-local terms in the effective action of gravity theories.
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