Abstract
Static, spherically symmetric black hole solutions to the semi-classical Einstein equation are studied, including the effect of the quantum energy-momentum tensor for conformal matters with 4D Weyl anomaly. Through both perturbative and non-perturbative methods, we show that the quantum effect can play a crucial role in shaping the nearhorizon geometry, and that the existence of the horizon requires fine-tuning.
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Ho, PM., Kawai, H., Matsuo, Y. et al. Back reaction of 4D conformal fields on static black-hole geometry. J. High Energ. Phys. 2018, 56 (2018). https://doi.org/10.1007/JHEP11(2018)056
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DOI: https://doi.org/10.1007/JHEP11(2018)056